The galaxy presents a roughly elliptical morphology, elongated along its major axis. A bright, concentrated central bulge dominates the galaxy's luminosity profile. The bulge exhibits a smooth, featureless appearance. Fainter, diffuse light extends outward from the central bulge, forming a disk-like structure. However, the disk component appears poorly defined, with no readily apparent spiral arm structure.

The galaxy's color gradient suggests a higher concentration of older stellar populations within the central bulge, indicated by a redder hue. The outer disk appears bluer, potentially indicating the presence of younger, hotter stars, though the overall color is still moderately red. No signs of active galactic nuclei features are apparent. Possible minor tidal distortions appear on one side of the galaxy, indicating a past or ongoing interaction. 
