The galaxy presents as a fairly smooth, elliptical structure with a concentrated central bulge that appears yellowish. There are no prominent spiral arms or dust lanes visible. The overall shape is mostly round. The color suggests an older stellar population with lower rates of current star formation, consistent with a lack of blue light usually associated with younger, hotter stars. There is no evidence of any major ongoing mergers or significant tidal disturbances in the immediate vicinity. A slight asymmetry may suggest minor interactions or internal dynamics. The outer regions of the galaxy fade gradually into the background, indicating a smooth transition in stellar density.
