The galaxy exhibits a generally elliptical morphology, appearing largely smooth and lacking prominent spiral arms or a distinct disk structure. The light is concentrated towards the center, indicating a significant bulge component. There is a color gradient present, shifting from a yellowish-white core to a slightly bluer hue in the outer regions. No strong signs of ongoing major mergers or significant tidal disturbances are evident in this image, suggesting a relatively settled structure, though subtle asymmetries may hint at past minor interactions. Based on the colors, the core likely contains an older stellar population, while the outer regions may have experienced more recent, albeit limited, star formation.
