The galaxy presents as an elliptical-like morphology with a moderate degree of roundness, appearing slightly elongated. The central region exhibits a concentrated, relatively smooth luminosity profile, indicative of an older stellar population and a spheroid-dominated structure. There are no clear spiral arm features. Faint, diffuse outer regions suggest a gradual decline in stellar density away from the center. There is a slight asymmetrical nature to the light distribution, with a more pronounced extension in one direction, which may be indicative of a past minor merger or tidal interaction. Overall color is slightly redder, suggesting older stars and less active star formation.
