The galaxy appears to be an elliptical galaxy, characterized by a smooth, centrally concentrated light distribution. Its overall shape is elongated, exhibiting a clear major axis and a smaller minor axis. The light profile suggests a high Sersic index, indicative of a de Vaucouleurs profile often seen in ellipticals. The galaxy's core region displays a bright, yellowish hue, possibly indicating an older stellar population dominating this area. There is little to no visible evidence of spiral arms or significant dust lanes. Faint, diffuse light extends outwards from the core, gradually fading into the background sky. The overall morphology suggests a relatively evolved, passively evolving galaxy with a significant bulge component. There is no apparent sign of any recent or ongoing major merger activity, although the overall distribution is slightly disturbed, suggesting minor interactions may have occurred.
