The galaxy presents as an elliptical morphology, with a smooth, concentrated central bulge. The overall color is reddish-yellow, suggesting a population of older stars and a relative lack of ongoing star formation, particularly within the central region. There is minimal evidence of spiral arms or significant dust lanes. The light distribution is fairly uniform, showing a gradual decrease in intensity from the core outwards, consistent with a high Sersic index. A slight elongation is observed, hinting at a mild degree of flattening. A small region of redder color is visible close to the core, possibly indicating a small region of dust or red giant stars. The galaxy appears relatively undisturbed, showing no strong signs of tidal interactions or recent mergers, appearing as a relatively isolated system.
