This galaxy presents as a somewhat diffuse, centrally concentrated object. The overall morphology appears largely spheroidal, lacking prominent spiral arms or a well-defined disk structure. There is a suggestion of subtle internal features, perhaps slight asymmetries or irregularities in the light distribution.

The color profile indicates a potentially complex stellar population. The central region displays a bluer hue, potentially indicative of younger, hotter stars or ongoing star formation in this region. The outer regions show a slight reddening, suggesting a population of older, redder stars. Overall, the galaxy does not appear intensely star-forming, but some level of activity may be occurring within the core.

There's no clear evidence of a significant tidal interaction or recent merger, although the slight irregularity in its shape could potentially point to a minor disturbance. More detailed analysis would be required to confirm whether the features are related to internal processes or external influences. The size suggests it is a galaxy of substantial dimensions.
