The galaxy appears to be a relatively bright, slightly elongated object. Its light is concentrated towards the center, indicating a significant bulge component. The central region exhibits a yellow-white hue, which is indicative of an older stellar population dominating the core. A faint, diffuse halo extends outward from the central bulge, displaying a bluer tint relative to the core. This suggests the presence of younger, hotter stars in the outer regions, or the galaxy may have a disk component with more active star formation there. There are no clear indications of spiral arm structures. The overall morphology suggests an intermediate type galaxy, possibly between an elliptical and a spiral galaxy. There are no obvious signs of recent major merger events.
