The galaxy presents as a relatively smooth, elliptical-like structure. Its light profile appears centrally concentrated, with a gradual decrease in brightness outwards from the core. The galaxy appears to have a yellow to golden hue, with subtle hints of redder tones, suggesting an older stellar population. There is a noticeable lack of distinct spiral arm structures or prominent dust lanes. The overall form appears generally undisturbed, with no strong signs of tidal features or major mergers. The galaxy exhibits a moderate degree of ellipticity, appearing more elongated than perfectly circular. The galaxy appears relatively isolated, with no immediately obvious companion galaxies in close proximity or signs of ongoing interactions. 
