This galaxy exhibits a generally elliptical morphology, appearing smooth and largely featureless. The light distribution suggests a high degree of radial symmetry, with the intensity gradually decreasing from the core outwards. There is no apparent evidence of spiral arms or a distinct disk structure.

The color gradient is subtle but present. The central region appears slightly more reddish-orange, transitioning to a bluer halo surrounding the core. This might indicate an older stellar population concentrated in the center, with younger, bluer stars further out.

There is no indication of any major ongoing merger activity or significant tidal disturbances. Minor irregularities in the outer regions might suggest the presence of smaller interactions or past accretion events, but they do not drastically alter the overall smooth appearance of the galaxy. The galaxy's size is moderate, neither exceptionally large nor particularly compact.

Given the overall characteristics, this galaxy likely belongs to the early-type classification, possibly an elliptical or lenticular galaxy. Further spectroscopic data would be useful to confirm its stellar population and star formation history.
