The galaxy presents as an elliptical or lenticular system with a smooth, largely featureless morphology. The light profile shows a central concentration with decreasing intensity outwards, with a noticeable yellow hue in the core which may indicate an older stellar population. A slightly bluer halo surrounds the core region, suggesting the presence of some younger stars or ongoing star formation, although the rate appears to be relatively low. The overall shape is mostly round, with a minor elongation. There is no obvious sign of spiral arm structure or a prominent dust lane. The galaxy appears relatively undisturbed, lacking any significant tidal features or indications of a recent major merger event, however there might be minor disturbances.
