The galaxy presents as a flattened elliptical, though exhibiting some disk-like characteristics. The central bulge is bright and appears yellowish, indicative of an older stellar population. Moving outwards from the core, the galaxy exhibits a fading blue hue in the disk, suggesting the presence of some younger, hotter stars. The overall structure is fairly smooth, with only minor irregularities or disturbances visible. There is a slight elongation to the galaxy's shape, tending toward a cigar shape. There are no clear indications of any major ongoing mergers, though some minor tidal disturbances might be present. Star formation appears to be minimal to non-existent.
