The galaxy presents a somewhat elliptical morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards the outer regions. The color profile appears to be relatively uniform, with a dominant yellowish hue, suggestive of an older stellar population. There is a secondary light concentration nearby that may be tidal debris, a satellite galaxy, or a background object. Overall, the image suggests the galaxy is an early-type system, potentially undergoing minor interactions.
