The galaxy presents an elliptical morphology, with a high degree of smoothness across its structure. The light distribution appears centrally concentrated, exhibiting a bright, well-defined core. The isophotes transition smoothly from the central region outwards, and the galaxy shows a gradual decline in surface brightness towards its outer edges. The shape is neither perfectly circular nor significantly elongated, residing more towards an intermediate elliptical classification. There are no visible signs of spiral arms, bars, or significant dust lanes. There is also no evidence of any tidal disturbances or ongoing mergers, with the overall structure appearing regular and undisturbed. The galaxy exhibits a yellow hue, suggestive of a stellar population dominated by older stars.
