The galaxy presents a generally smooth, elliptical morphology. There is a central, bright bulge that dominates the overall structure. The light profile appears centrally concentrated, with a gradual decrease in intensity extending outwards. The color appears relatively uniform throughout the galaxy, with a slightly redder hue in the central region, suggesting an older stellar population. There is a lack of any distinct spiral arm structure or significant dust lanes, contributing to its smooth appearance. The galaxy appears to be relatively isolated, showing no strong signs of tidal interactions or ongoing mergers with other galaxies, though there is a possible slight disturbance on the periphery.
