The galaxy presents as a relatively smooth, elliptical-like object. It has a concentrated, bright core with a diffuse halo extending outwards. The color is generally yellowish-orange, potentially indicating an older stellar population and/or the presence of dust. No prominent spiral arms or distinct disk features are discernible. The galaxy's shape appears mostly round, showing only minor deviations from perfect circularity. There is no clear evidence of any major ongoing mergers, though a slight asymmetry on one side could be indicative of a minor interaction or disturbance. The overall appearance suggests a quiescent galaxy with a low star formation rate.
