The galaxy exhibits a primarily smooth morphology, with a hint of disk-like structure. The central region appears brighter and more concentrated, suggesting a significant bulge component. The galaxy displays an overall rounded shape, tending toward elliptical, with a very slight elongation. The color profile indicates a redder core region, possibly indicative of an older stellar population, transitioning to slightly bluer hues in the outer regions, suggestive of some ongoing star formation. There is evidence of a minor gravitational disturbance or interaction, possibly with a smaller companion galaxy, which might be influencing the observed morphology.
