The galaxy presents a mostly smooth, rounded morphology, with a noticeable central bulge dominating its structure. The color profile suggests an older stellar population, exhibiting a yellowish hue. There is some indication of a potential tidal feature or minor disturbance extending from the central region, possibly suggestive of past interactions or merging activity. Star formation appears to be relatively quiescent within the galaxy, as indicated by the lack of prominent blue regions typically associated with young, hot stars. The galaxy appears somewhat luminous. 
