The galaxy presents as an elliptical morphology, with a smooth, largely featureless appearance. It exhibits a concentrated central bulge which is bright and yellowish-white in color, suggesting a population of older stars. The outer regions of the galaxy fade gradually into the background, indicating a diffuse halo or envelope of stars. There is little evidence of spiral arms or dust lanes. Overall, this galaxy appears to be a well-formed, mature system with minimal recent star formation activity. There is some very minor disturbance in the symmetry of the light distribution, but it is not significant enough to suggest an ongoing merger.
