The galaxy presents as a lenticular or an elliptical galaxy based on its shape. It appears to be relatively smooth with no obvious spiral arm structure. There is a slight elongation. The color gradient suggests a concentration of older stars towards the center, indicated by the reddish hue in the core. The outer regions exhibit a bluer tint, potentially indicating a younger stellar population or some low-level ongoing star formation. There is no clear sign of a strong dust lane or a recent major merger event. The shape of the galaxy is generally regular, without significant distortions or tidal features.