The galaxy exhibits a largely smooth morphology with a high degree of central concentration. The light profile suggests a spheroid-dominated system, likely an elliptical galaxy. The overall color appears to be reddish-yellow, which is consistent with a stellar population dominated by older, redder stars. There is little evidence of spiral arms, dust lanes, or ongoing star formation. The galaxy appears to be relatively isolated, with no obvious signs of tidal interactions or recent mergers. The roundness suggests the galaxy is not a disk, but a more spherical shape.
