The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a high concentration of light, appearing bright and somewhat unresolved. The overall shape is more rounded than elongated. There is a slight asymmetry with a minor disturbance, possibly indicative of a weak tidal interaction. The color suggests a population of older stars, but there is also evidence of ongoing star formation. The galaxy appears relatively isolated, with no other obvious galaxies involved in a major merger, although there is some slight disturbance to the system.