The galaxy appears as a centrally concentrated object, with a fairly smooth and regular overall morphology. There is no strong evidence of spiral arm structure or a pronounced disk. The light is dominated by a reddish-yellow hue, suggesting a stellar population that is older and likely less actively forming stars. There might be a very faint, diffuse halo extending slightly beyond the bright central region, but the signal is weak. The general shape is fairly elliptical, closer to in-between and not perfectly round or cigar shaped. There are no obvious signs of any major interactions or ongoing mergers, though minor disturbances can’t be ruled out.
