The galaxy presents an elliptical morphology, appearing as a somewhat elongated spheroid. The central region exhibits a concentrated, bright, and yellowish hue, indicative of an older stellar population. The outer regions of the galaxy display a gradual decrease in luminosity, with a bluer tint, suggesting the presence of younger stars, although these are not the dominant features. The galaxy appears relatively smooth in texture with some features, with no distinct spiral arms or prominent dust lanes visible. There is no obvious evidence of recent major merger activity. The overall structure is consistent with an early-type galaxy undergoing moderate star formation.
