The galaxy presents as a concentrated central bulge with a surrounding disk-like structure, though the disk appears relatively smooth and featureless. The core exhibits a yellowish-white hue, potentially indicating an older stellar population. The outer regions of the disk display a faint bluish tint, suggesting the presence of some younger, hotter stars and ongoing star formation. The shape is generally elliptical, moderately elongated along its major axis. No prominent spiral arms or bar structures are visible. There is no obvious evidence of major tidal disturbances or ongoing mergers, although the slight asymmetry could suggest minor interactions or internal activity. The galaxy is moderately bright, suggesting a relatively high mass and luminosity. 
