The galaxy appears as a generally smooth and rounded object with a concentrated central bulge. The light distribution suggests an elliptical morphology, although some slight distortion might be present in the outer regions of the halo. The galaxy exhibits a color gradient, appearing slightly more yellow towards its center. This indicates an older stellar population is dominant, with potentially ongoing, low-level star formation activity. The galaxy appears relatively isolated with no strong indications of recent or ongoing major mergers, although minor tidal disturbances may be present. The halo is diffuse and not sharply defined, suggesting a gradual decrease in stellar density with increasing radius from the galactic center.
