The galaxy appears to be a relatively smooth, elliptical galaxy. It presents a centrally concentrated luminosity profile, indicative of an older stellar population. The galaxy exhibits a generally round morphology, lacking any prominent disk-like features or spiral arms. There is no obvious indication of tidal tails or strong distortions, suggesting no recent major merger events. Subtle color gradients are present, with a slightly yellower hue towards the center, potentially due to the presence of older, redder stars dominating the core. A faint, diffuse halo surrounds the galaxy, gradually fading into the background sky. The galaxy displays a blue tint, potentially indicating some relatively recent star formation, although the smooth morphology is not characteristic of star forming galaxies.
