The galaxy presents as a relatively smooth, elliptical structure. The light profile appears centrally concentrated, with a gradual decrease in intensity towards the outer regions. The major axis is noticeably longer than the minor axis, indicating a non-spherical shape. There may be a slight warp or disturbance in the morphology, but it is mostly composed of smooth light. The galaxy has colors skewed toward the redder end of the spectrum. It exhibits a central reddish core, with bluer hues present in the outer disk, which may indicate ongoing star formation. There is no evidence of a major ongoing merger, although the disturbed morphology may be suggestive of a minor interaction in the past.
