The galaxy presents as a centrally concentrated elliptical morphology with a smooth light distribution. The core region exhibits a yellowish-orange hue, suggestive of an older stellar population. A faint, diffuse halo extends outward from the central bulge, fading into the background. The overall shape appears somewhat round, with only a minor deviation from a perfect circular form. There is no visible evidence of spiral arms, dust lanes, or other prominent features typically associated with disk galaxies. No significant merger activity or tidal disturbances are apparent in the immediate vicinity.
