The galaxy presents a generally smooth and somewhat elliptical morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards the outer regions. The color appears to be relatively uniform across the galaxy, with a suggestion of a slightly redder hue. There is very little, if any, evidence of spiral arm structure or significant dust lanes. The galaxy appears to be relatively undisturbed, with no obvious signs of ongoing major merger activity, though a very subtle asymmetry may indicate minor interactions. The overall appearance indicates a galaxy dominated by an older stellar population, with a low rate of current star formation.
