The galaxy presents as a relatively smooth, elliptical-shaped structure with a noticeable central bulge. The core region exhibits a concentrated yellowish-orange hue, suggestive of an older stellar population. Progressing outwards from the core, there is a diffuse, greenish-yellow halo, potentially indicating a region of ongoing or recent star formation, albeit at a subdued rate. There is no apparent spiral arm structure or significant dust lane obscuration visible. The galaxy appears largely undisturbed, lacking any obvious signs of major mergers or tidal interactions. It has a generally even color distribution that indicates low levels of disturbance. Overall, the galaxy appears to be an evolved system with moderate mass and only minor activity in star formation.
