The galaxy presents as a relatively compact and luminous system. Its overall morphology appears to be that of a disk galaxy, but the image resolution limits detailed classification. It displays a central bulge that appears yellow-white in color. The bulge seems to smoothly transition into a bluer, diffuse disk structure. No distinct spiral arms are readily apparent. The disk component exhibits mottling, possibly indicative of active star formation regions or dust lanes, though again, image resolution limits detailed analysis. The galaxy appears moderately inclined with respect to our line of sight. There is no obvious evidence of major mergers or tidal disturbances, although some minor asymmetry in the outer regions of the disk cannot be ruled out. 
