The galaxy presents an elliptical morphology, displaying a smooth, centralized concentration of light. There is a gradual decline in luminosity from the core outwards, with no apparent spiral arm structures or prominent dust lanes visible. The color profile suggests an older stellar population, as indicated by the yellowish hue, consistent with a lower rate of ongoing star formation activity. There is a slight asymmetry visible that may suggest a past or ongoing minor disturbance. The galaxy appears well-defined and relatively isolated.
