The galaxy presents as a relatively smooth, elliptical form. Its overall shape is somewhat elongated, with the major axis extending more prominently than the minor axis, suggesting a classification somewhere between round and cigar-shaped. The light distribution is concentrated towards the center, with a gradual decrease in brightness towards the outer edges. The galaxy appears to lack prominent spiral arm structures or significant dust lanes. There is minimal evidence of recent or ongoing major mergers or strong tidal disturbances. The morphology is consistent with a spheroidal galaxy, potentially an elliptical. 
