The galaxy presents a generally elliptical morphology, though it is not perfectly round. The light distribution appears relatively smooth, with a high concentration toward the center which seems to be a yellow-ish color, indicating older stars. From this central region, the light gradually fades outwards. The galaxy displays a slight disc-like appearance with only subtle internal features or spiral structure visible. There may be a slight disturbance or interaction occurring, as suggested by the asymmetry in its outer regions, but not a complete merger event. Overall, the galaxy seems to be moderately massive with a relatively low rate of star formation.
