The galaxy presents as a disk-shaped system, inclined somewhat to our line of sight. It exhibits a prominent central bulge, appearing yellowish, which likely indicates an older stellar population concentrated in the core. Fainter spiral arm structures extend from the central region, showing a bluer hue suggestive of ongoing star formation. The dust lanes within the disk are not clearly visible. The galaxy appears relatively isolated, without strong visual evidence of major mergers or significant tidal distortions, although minor disturbances cannot be ruled out.
