The galaxy presents as a centrally concentrated object with a generally smooth morphology. It exhibits an approximately elliptical shape, tending towards round. The galaxy's color profile indicates a relatively older stellar population, appearing predominantly yellow-reddish. No distinct spiral arms or strong dust lanes are discernible. There is no indication of a major ongoing merger event; however, the possibility of a minor tidal disturbance cannot be completely ruled out, though it is not immediately apparent. The light is evenly distributed, indicative of a lack of significant star formation within its structure.
