This galaxy exhibits an elliptical morphology, appearing mostly smooth with a slight elongation. There is evidence of an ongoing or recent merger event, indicated by the presence of two distinct, luminous concentrations within the galaxy's halo. The primary component appears somewhat spheroidal. The color indices suggest the presence of an older stellar population, with a reddish hue dominating the light emitted from this system. There may be a faint tidal tail or other disturbance hinting at gravitational interaction. Overall, this galaxy appears to be a massive system in a relatively advanced stage of its evolution.
