The galaxy presents as a relatively compact, elliptical-like structure. It exhibits a smooth, diffuse light distribution, lacking any prominent spiral arms or distinct features that would suggest active star formation on a large scale. The color profile indicates a concentration of older stellar populations, seen in the slightly redder hue toward the central region, with a faint blue hue that gradually fades with distance from the center. No obvious signs of tidal interactions or mergers are visible. Based on the overall appearance, it is potentially an early-type galaxy with minimal current star formation.
