The galaxy presents a generally smooth, elliptical morphology. The light distribution is centrally concentrated, exhibiting a bright core that gradually diminishes in intensity towards the outer regions. There is minimal evidence of spiral arm structures or prominent dust lanes, suggesting that it is a relatively evolved system. The galaxy appears slightly elongated, with an apparent axis ratio suggesting a mild degree of ellipticity. Based on the color indices, the galaxy exhibits colors consistent with a population of older stars, with a notable contribution from redder wavelengths. The overall appearance suggests a relatively quiescent galaxy with little ongoing star formation. There is a possible indication of a very minor disturbance in its symmetry, although it is not clear if this is tidal in nature.
