The galaxy presents as a centrally concentrated elliptical morphology with a smooth, diffuse light distribution. The core appears to be luminous and slightly elongated, transitioning gradually outwards to a fainter halo. There is no apparent dust lane, spiral arm structure, or nuclear activity visible in this image. The galaxy exhibits a slightly off-white color, hinting at an older stellar population. Close inspection reveals a subtle unevenness to the outer halo, possibly indicative of minor tidal interactions or past accretion events. The overall form suggests a galaxy nearing the end-stage of its evolution.
