The galaxy appears to be an elliptical or lenticular type, exhibiting a smooth, centrally concentrated luminosity profile. There is a slight elongation observed, with the major axis perhaps twice the length of the minor axis. The core region exhibits a reddish-orange hue, suggesting an older stellar population and minimal ongoing star formation. This color gradually fades to a slightly bluer tint towards the outskirts, though the overall color remains redder than typical spiral arms. There is no distinct disk structure or spiral arm features that are readily apparent. No signs of active galactic nucleus activity are detected in this imagery, nor is there any evidence of a strong tidal interaction or a recent merger event. It is likely a massive galaxy due to its consistent color, even luminosity, and large size.
