The galaxy appears as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that is yellowish-orange. The light gradually fades from the core towards the outer regions, suggesting a decrease in stellar density with increasing radius. There is very little evidence of spiral arms or distinct features, such as dust lanes or active star-forming regions. The overall morphology points toward an early-type galaxy. Based on color, it is likely composed of an older stellar population, potentially indicating low current star formation. There are no visible signs of significant tidal disturbances or ongoing mergers.
