The galaxy presents as a moderately luminous object, exhibiting a generally smooth morphology. The overall shape appears largely elliptical, with a notable concentration of light towards the central region. The color profile suggests an older stellar population, indicated by the redder hue. There is a potential interaction or merger occurring, as evidenced by two distinct bright clumps within the galaxy's structure. The relative smoothness and roundness suggests it has undergone or is undergoing the process of becoming a smooth elliptical galaxy through a possible merger. Some minor disturbances are noted, suggesting potential tidal interactions, or ongoing gravitational perturbations. There is a low likelihood of ongoing, major merging activity and a moderate chance of a merger being in progress. The overall mass is significant, contributing to the gravitationally bound structure. Low star formation rates are indicated by the overall color and smooth morphology.
