The galaxy presents as a smooth, elliptical-like structure, exhibiting a concentrated central bulge. The light profile appears relatively uniform, with a gradual decrease in intensity moving outwards from the core. The isophotes are moderately elliptical. Color gradients are subtle, with the central region displaying a slightly yellower hue, indicative of an older stellar population. The outer regions show hints of bluer tones, suggesting the presence of some younger stars, although star formation appears generally quiescent. There are some apparent minor structural irregularities, possibly suggesting a past minor interaction or disturbance. The galaxy exhibits no prominent spiral arm structures or significant dust lane obscuration. It is intermediate in size.
