The galaxy presents a morphology consistent with an elliptical or lenticular galaxy. It exhibits a smooth, centrally concentrated luminosity profile, with a diffuse halo fading into the background. The major axis appears slightly elongated, suggesting a deviation from a perfectly spherical shape. There is evidence of some asymmetrical features, potentially indicating minor disturbances or ongoing interactions. A faint disk-like structure might be present, although it is not clearly defined. The overall color suggests a population of older stars. The system appears relatively isolated with no obvious major mergers occurring. There are areas of blue and orange-red that suggest some star formation or mergers, but the system is still primarily an older system.