The galaxy appears to be a relatively large, well-defined elliptical galaxy at a considerable distance. Its overall shape is elongated, tending towards a cigar-like morphology. The light distribution is smooth and centrally concentrated, with the highest intensity emanating from the core region. The core itself is not clearly resolved.

A distinct color gradient is observed, with the central regions appearing more yellow/orange, indicative of an older stellar population. The outer regions are fainter and tend towards redder hues. There are suggestions of minor disturbances or asymmetries within the halo, but the galaxy appears largely undisturbed, with no evidence of major mergers or tidal interactions. The disk component is very subdued. It is likely a high mass galaxy, where the star formation is low.
