The galaxy appears as a relatively compact, elliptical-like structure with a smooth light distribution. There is a slight elongation observed, trending towards a cigar shape. The color profile suggests a population of older stars, skewed towards the redder end of the spectrum. Evidence suggests a possible merger event, or at least a minor gravitational disturbance, as the galaxy's shape is slightly irregular. The galaxy is not perfectly round, as it has an in-between roundness. There may be an ongoing, albeit weak, star formation activity based on its color profile.