The galaxy presents as a moderately luminous, elliptical morphology. A concentrated, bright central bulge region dominates the galaxy's overall structure, fading gradually outward into a less defined halo. The smooth texture suggests a relatively old stellar population. The overall color appears slightly redder in the central regions, possibly indicating a greater concentration of older, redder stars. The outer regions exhibit a bluer hue, hinting at the presence of younger stars or ongoing star formation, although at a low rate. The galaxy shows a slight degree of flattening, leaning towards an oblate shape, but it does not exhibit any obvious spiral arm structures or significant dust lanes within the observed image. No major mergers or strong tidal disturbances are immediately apparent, the overall appearance suggests a relatively undisturbed galaxy.
