The galaxy presents as an elliptical morphology, characterized by a centrally concentrated luminosity profile that gradually decreases outwards. The color index suggests a population of older stars, indicative of reduced recent star formation activity. The galaxy appears relatively undisturbed, lacking prominent tidal features or morphological irregularities, though a slight asymmetry might be present, potentially signaling a minor interaction in its past or a subtle internal structure. Overall, it appears as a relatively smooth and evolved system.
