The galaxy presents a generally smooth morphology, with a possible slight ellipticity. The overall light profile appears relatively centrally concentrated. There's a suggestion of some substructure or slight irregularity within the galaxy's profile, but it's largely blended into a smooth distribution. The galaxy's color appears moderately red, suggestive of an older stellar population and/or significant dust content. No obvious spiral arms or strong star-forming regions are visible. There is no clear evidence of a recent or ongoing major merger event. However, based on the image alone, the possibility of minor disturbances cannot be ruled out.