The galaxy presents as a slightly elongated, roughly elliptical structure. The central region exhibits a bright, concentrated core, suggestive of a dense stellar population. A gradual decrease in luminosity is observed moving outward from the core, forming a relatively smooth halo. There appears to be a subtle disk, not well defined, but noticeable due to a slight flattening of the galaxy. Faint hints of possible minor disturbances or tidal features are present, though not prominent enough to conclude an active merger event. The color gradient shows a yellowish-white center, with outer regions exhibiting a slightly bluer hue, possibly indicating the presence of younger stars in the disk. Overall, the galaxy appears to be relatively evolved and quiescent.
