The galaxy presents as a centrally concentrated system with a smooth overall appearance. There is a noticeable increase in luminosity towards the center, suggesting a bright nucleus or bulge. The galaxy exhibits a relatively rounded shape with a slight elongation. There is no obvious spiral structure or prominent disk. Faint extensions or halos are present, but do not show any signs of tidal disruption, suggesting no recent major merging events. The overall color appears moderately red, suggesting an older stellar population and/or significant dust content.
