The object appears to be a lenticular or elliptical galaxy, exhibiting a smooth, concentrated light profile. It presents an elongated, cigar-shaped morphology. The central region displays a yellow-orange hue, suggestive of an older stellar population. Moving outwards from the core, the galaxy fades into a bluer colour. The light is evenly distributed, lacking any signs of spiral arms or distinct features and there is no evidence of a recent merger, strong tidal interactions, or significant star formation. Overall, the galaxy seems to be a relatively quiescent system composed of mostly old stars with a substantial mass.
