The galaxy presents as a largely featureless, elliptical form. Its light profile is characterized by a bright, concentrated core that gradually fades into a diffuse halo. The overall color appears to be slightly redder, suggesting an older stellar population and a relatively low rate of current star formation. The smoothness of the light distribution indicates minimal dust lanes or spiral arm structures. There is no obvious evidence of tidal disturbances or ongoing mergers, suggesting it is a relatively relaxed system. The galaxy exhibits a moderately high luminosity. Its apparent size suggests that it is a relatively small galaxy. The elliptical shape is well-defined, with no significant deviations from axisymmetry. The galaxy's morphology is consistent with that of an early-type galaxy, likely an elliptical galaxy.
