The galaxy presents as a flattened, elliptical morphology with a smooth, diffused light profile. The central region appears brighter and more concentrated with an ochre hue, suggestive of an older stellar population. Moving outwards from the center, there appears to be a gradual decrease in luminosity and a shift toward slightly bluer tones. This might indicate the presence of some younger stars in the outer regions, though star formation is not obviously prominent. There are suggestions of a very faint, disk-like structure, but the galaxy is dominated by its elliptical shape. There are no obvious signs of spiral arms, bar structures, or a recent major merger event. The galaxy's shape falls between being perfectly round and cigar shaped, tending towards the round end.
