The galaxy presents a primarily smooth, elliptical morphology with a central bulge dominating the structure. The light distribution appears relatively uniform, lacking prominent spiral arms or distinct features. There is a slight elongation to the galaxy's shape, tending towards a more rounded appearance. A subtle color gradient is observed, with the central region exhibiting a yellowish hue, potentially indicating an older stellar population, while the outer regions display bluer tones, perhaps due to the presence of younger stars. No significant signs of ongoing major mergers or tidal disturbances are apparent, although some minor irregularities may suggest weak interactions or internal processes. Overall, the galaxy appears to be a relatively quiescent system, exhibiting characteristics consistent with a moderately massive galaxy with a low star formation rate.
