The galaxy presents as a single, unresolved object with a generally elliptical morphology. The light distribution appears smooth, with a high degree of central concentration. The core region exhibits a yellow-white hue, suggesting an older stellar population. The galaxy lacks any obvious spiral arm structures, bars, or other prominent features typically associated with disk galaxies. The light tapers off gradually from the core, without any distinct edges, indicative of a diffuse stellar halo. Faint reddish tones are present in the outer regions, possibly indicating a population of cooler, older stars. There's no clear evidence of dust lanes or significant ongoing star formation. Overall, it has the appearance of an elliptical galaxy at a significant distance.
