The galaxy appears as a single, relatively smooth object with a concentrated central bulge. The light distribution is generally elliptical with a high degree of circularity. There is a notable lack of distinct spiral arms or significant features indicating ongoing mergers. A faint disk may be present and contributes to the galaxy's observed size. The galaxy exhibits a color gradient, with the central region appearing more yellow-orange, suggestive of an older stellar population, while the outer regions show a slightly bluer tint, potentially indicating the presence of some younger stars. Overall, the galaxy's morphology indicates a system dominated by an evolved stellar population with a suppressed rate of star formation and a substantial mass.
