The galaxy presents as a single, concentrated object with a predominantly smooth light distribution. The morphology suggests a likely elliptical classification, exhibiting a high degree of circular symmetry. There is minimal evidence of spiral arm structures or significant disk features. The galaxy appears reddish-orange, indicative of a stellar population dominated by older, redder stars, with minimal ongoing star formation. Any faint blue regions may be indicative of some star formation. No tidal tails, bridges, or other signs of ongoing or recent merger activity are distinctly visible. Based on the light profile, the galaxy seems to be relatively compact.
