The galaxy presents as a centrally concentrated system with a smooth, diffuse morphology. It appears elliptical in shape, lacking any distinct spiral arm structure or prominent dust lanes. The core is bright and concentrated, suggesting a high density of stars in the central region. There is a radial color gradient, transitioning from a yellowish-white hue at the core to a more reddish color in the outer regions. This could indicate an older stellar population dominating the outer parts of the galaxy. The galaxy appears relatively isolated, showing no obvious signs of tidal interactions or ongoing mergers, though a very small, faint irregular feature may be present nearby. The overall smooth appearance suggests that the galaxy is likely a relatively evolved system.
