The galaxy presents as a moderately luminous, elongated spheroid. Its color profile suggests a greater concentration of older stars, giving it a yellowish hue. The light is relatively smooth and centrally concentrated, lacking any prominent spiral arm structures or significant dust lanes. Its shape suggests a classification leaning towards an elliptical or lenticular type. The galaxy exhibits some degree of asymmetry, possibly indicating a past or ongoing minor interaction. No prominent tidal tails or strong distortions are visible. The core region appears brighter, but it is not clearly resolved. The overall appearance suggests that the object is a well-evolved system with low ongoing star formation.
