The galaxy presents as a relatively smooth, centrally concentrated object with a spheroidal morphology. The light distribution is dominated by a bright, yellowish core that likely indicates an older stellar population. Moving outwards from the core, the color becomes slightly bluer, possibly indicative of a younger stellar population in the outer regions. There is no apparent disk structure, spiral arms, or significant dust lanes visible in the image. The outer edges of the galaxy appear diffuse and indistinct, blending into the background sky. There is no indication of any major mergers or tidal disturbances present. The galaxy is fairly circular in shape with a round appearance.
