The galaxy presents as a relatively smooth, elliptical structure. The central region exhibits a concentrated, bright luminosity with an orange-yellow hue, suggestive of an older stellar population. The luminosity gradually decreases from the center outwards. There is very little indication of spiral arm structure or significant dust lanes. The outer regions of the galaxy appear more diffuse and exhibit a slightly bluer tint, possibly indicating the presence of some younger stars, although the dominant color suggests a galaxy in which star formation is suppressed. The overall shape approximates a rounded form, leaning toward a more circular morphology, with no obvious signs of tidal disturbances or ongoing major mergers. Possible minor disturbance or close interactions cannot be ruled out, though the galaxy appears largely undisturbed.
