The galaxy presents as an elliptical morphology, exhibiting a smooth, diffuse light distribution. The core region displays a high surface brightness, gradually decreasing towards the outer edges. The axial ratio indicates that the galaxy is somewhat flattened. The observed color gradient suggests a redder color in the central bulge, possibly indicating an older stellar population, with the outer regions exhibiting a slightly bluer hue, which may suggest the presence of younger stars, albeit at low rates. There is no apparent spiral arm structure or prominent dust lanes visible within this galaxy, suggesting a more evolved system with potentially quenched star formation. Tidal features are absent, suggesting no recent major merger events. Overall, the galaxy appears to be an intermediate-sized system with a generally smooth appearance.
