The galaxy presents as a moderately sized object with a relatively diffuse structure. The light distribution is concentrated towards the center, exhibiting a gradual decrease in intensity outwards, suggesting a central bulge component. 

The galaxy's color profile is notably redder in the central region, transitioning to a bluer hue towards the outer edges. This color gradient may indicate a difference in stellar populations, with older, redder stars dominating the core and younger, bluer stars populating the outer disk or spiral arms.

Morphologically, the galaxy appears largely smooth, hinting towards an elliptical galaxy classification, but there is a slight hint of a disk-like structure. Subtle asymmetries or irregularities are visible, potentially indicating past or ongoing interactions or minor mergers. These disturbances appear minor.
