The galaxy appears as a somewhat elliptical structure, exhibiting a smooth, concentrated central bulge. A fainter, extended halo surrounds the central region. The color profile suggests a relatively evolved stellar population, trending toward redder hues, particularly within the core. There appears to be little evidence of active star formation from the color and morphology alone, indicating a galaxy that is likely quiescent. There is no evidence of significant tidal disturbances or ongoing mergers within the galaxy's immediate vicinity, and the overall morphology appears relatively undisturbed. The galaxy appears to be relatively isolated in its location.
