This galaxy appears to be a relatively smooth, elliptical system. It exhibits a central bulge that appears slightly elongated, trending towards a cigar shape. There is no obvious presence of spiral arms or a distinct disk structure. The galaxy appears to be relatively undisturbed, without any major signs of ongoing mergers or tidal disruptions, only minor disturbances might be happening. The color profile suggests a population of older stars, with a higher concentration towards the redder end of the spectrum.
