The galaxy presents as a relatively smooth, elliptical structure with a slightly elongated shape. It exhibits a yellow-orange hue concentrated towards its center, suggesting an older stellar population dominating the core. Fainter, bluer tinges are visible towards the outer edges, hinting at the presence of younger, hotter stars or regions of ongoing star formation, albeit at a subdued level. The overall morphology indicates the galaxy is likely in a relatively quiescent state, without strong evidence of spiral arms or significant dust lanes. There may be some minor tidal disturbances present.
