The galaxy presents a generally smooth morphology. The central region exhibits a concentration of light, appearing somewhat round in shape, suggesting a possible bulge. There are hints of a diffuse disk structure surrounding the central bulge. The galaxy does not appear to be undergoing a major merger or significant tidal disruption based on its overall structure, though there are some minor asymmetry in the disk region that may be indicative of a minor disturbance. The color gradient suggests a population of older stars dominating the light output.
