The galaxy appears as a luminous, centrally concentrated object.  Its overall morphology suggests a spheroid, likely an elliptical galaxy, but further analysis would be required to confirm this. There is some indication of a minor, non-axisymmetric component to the light distribution, possibly a faint tidal feature or irregularity, although it could be an artifact. It displays a reddish hue, possibly indicating an older stellar population and suppressed star formation activity. The spatial extent seems relatively compact. There is no clear evidence of spiral arm structure or a prominent disk component.
