The galaxy presents as a relatively smooth, elliptical morphology. The central bulge exhibits a bright, concentrated luminosity gradient, indicating a high stellar density. Moving outward from the core, the luminosity decreases gradually, displaying a more diffuse stellar distribution. The galaxy appears slightly elongated, deviating minimally from a perfectly circular shape. There is evidence of minor internal disturbances or asymmetries in the light distribution, hinting at a possible interaction or past merger event. The overall color profile suggests a population of relatively old stars, although a small amount of recent star formation might be present.
