The galaxy presents as a relatively smooth, lenticular-like structure, potentially an elliptical galaxy transitioning into a more disk-dominated system. Its overall color profile suggests an older stellar population. The central bulge exhibits a yellowish-orange hue, indicating the presence of evolved stars. The outer regions appear somewhat bluer, hinting at ongoing, albeit possibly low-level, star formation, though this activity does not disrupt the galaxy's generally smooth appearance. A slight asymmetry or minor disturbance in the outer structure may suggest a past or ongoing interaction with a smaller companion, however the tidal disruptions do not suggest a major merger event. The galaxy shows an intermediate degree of roundness and does not appear to be either perfectly spherical or highly elongated. 
