The galaxy presents an elliptical morphology, appearing as a smooth, concentrated distribution of light with a noticeable central bulge. The galaxy's overall shape appears slightly elongated with a clear major and minor axis, approaching a more circular form. There appears to be a lack of distinct spiral arm structures and is relatively smooth, suggesting a more evolved stellar population. Color gradients are observed, with a central region displaying a yellowish-white hue, transitioning towards a bluer tint in the outer regions. This suggests a gradient in stellar populations, where older, redder stars are concentrated in the core, and younger, bluer stars are present in the outer disk. The galaxy exhibits a moderate degree of apparent brightness and the overall structure shows no obvious signs of major disturbances or ongoing mergers, though minor asymmetries might exist. The galaxy seems relatively isolated, without close companions visually evident.
