The galaxy presents as a moderately luminous, primarily smooth object, likely an elliptical or lenticular type. Its overall shape is neither perfectly spherical nor highly elongated, appearing somewhat in between. There is a slight indication of a flattened disk-like structure. There's no obvious spiral structure, and the light is concentrated in the central region, which suggests an older stellar population. There is no signs of any tidal tails or major morphological disturbances, suggesting the galaxy has not undergone a recent major merger event. The galaxy's color appears generally redder, which likely suggests a suppressed star formation rate and a relatively large stellar mass.
