The galaxy presents a largely smooth, elliptical morphology. Its color profile suggests a redder stellar population, indicative of older stars and a lack of significant ongoing star formation. The galaxy exhibits a generally round shape, with minimal deviation from a circular structure. While a smooth appearance dominates, subtle disturbances are present that may indicate a past or ongoing minor interaction with a smaller companion. These potential disturbances consist of slight irregularities in the outer regions of the galaxy. No spiral arm structures or other distinct features are visible.
