The galaxy presents as a relatively smooth, elliptical-like structure. Its light is concentrated towards the center, displaying a bright central bulge. The object exhibits a yellow-white hue in the central region that transitions to redder tones further from the core, suggesting an aging stellar population. The overall shape suggests a lack of significant ongoing star formation. There appears to be only a subtle hint of a disk structure. No clear signs of tidal disturbances or mergers are evident, and the galaxy appears relatively isolated in this field of view.
