The galaxy presents a generally smooth, elliptical morphology. The core region is bright and appears a yellowish-white color, indicative of an older stellar population. Moving outward from the core, the intensity of the light decreases gradually, transitioning into a less distinct and more diffuse halo. There is a subtle color gradient, with the outer regions showing hints of bluer hues, possibly indicating some pockets of younger stars. The overall shape appears fairly round. There is no obvious evidence of strong tidal features, merging activity, or a prominent disk structure. The light is largely centrally concentrated, and although it seems to have a small estimated effective radius, suggesting it is likely to be a compact object. The estimated mass suggests a relatively massive galaxy. Evidence suggests that star formation rate is relatively low.
