The galaxy presents as a centrally concentrated object with an overall elliptical morphology. The light profile appears relatively smooth, with no discernible spiral arm structures. The central region is characterized by a bright, diffuse glow, suggesting a high concentration of stars and possibly an active galactic nucleus. Some irregular features are present within the smooth light profile, which may indicate minor tidal disturbances or ongoing merger activity. The galaxy appears to be actively forming stars at a relatively slow rate. The estimated size indicates it is a moderate-sized galaxy. The object exhibits a color gradient, with the central region appearing more yellow, and the outer regions trending toward a bluer hue, potentially indicative of differing stellar populations or dust content. The morphology leans towards a round shape, although some elongation is observed. A significant fraction of its light appears to be emitted by older stellar populations.
