The galaxy presents as a single, concentrated object with a largely smooth morphology. It appears somewhat elliptical in shape, exhibiting a moderate degree of roundness, with the major axis only slightly longer than the minor axis. The central region displays a notable concentration of light, gradually decreasing towards the outer edges. The color profile suggests an aging stellar population. The core emits a reddish-yellow hue, potentially indicating the dominance of older stars. There is faint blue emission present in the outer edges of the galaxy. The galaxy does not display any major disturbances. There are no significant tidal tails or strong asymmetries visible. The light distribution appears relatively even. There are no visible signs of interaction with other galaxies or ongoing mergers.
