The galaxy appears to be an elliptical galaxy, characterized by a generally smooth and rounded morphology. It exhibits a centrally concentrated luminosity profile, with the brightest region located at the core. There is a slight extension around the brighter central region. The light distribution suggests a relatively high degree of spherical symmetry, with minimal evidence of spiral arms or a distinct disk structure. There's no apparent major ongoing merging activity, though there might be some minor gravitational disturbances. The galaxy's color is slightly redder, suggesting a relatively older stellar population. The galaxy appears relatively massive, with low star formation.
