The galaxy presents as a somewhat elliptical structure with a smooth, diffuse appearance. It exhibits a centrally concentrated luminosity profile, transitioning from a bright, yellowish-orange core to fainter, diffuse edges. The overall color suggests a population of older stars with little ongoing star formation. There is no discernible spiral structure or distinct features such as dust lanes or prominent star-forming regions. The galaxy's shape appears moderately flattened, and it shows no signs of any major recent merger activity or strong tidal disturbances, although a slight asymmetry hints at a possible minor interaction in its past.
