The galaxy presents as a relatively smooth, elliptical-like structure. It appears to be dominated by older stellar populations, judging by its overall color profile, exhibiting redder hues. There's a suggestion of a minor deviation from a perfect elliptical shape, with a subtle elongation. The central region is considerably brighter and more densely packed than the outer regions, implying a concentration of mass toward the core. There are no prominent dust lanes or spiral arm features discernible, lending support to classification as an elliptical or S0-type galaxy. It lacks any obvious signs of active galactic nuclei (AGN) activity or recent major mergers, although it displays minor disturbances.
