The galaxy presents as a relatively face-on spiral galaxy, albeit with a somewhat hazy appearance indicative of its distance. Its color gradient suggests a higher concentration of older stars toward the center, exhibiting a yellowish hue that transitions to bluer tones in the outer arms. While the spiral structure is apparent, the arms appear somewhat flocculent, lacking the grand design spiral structure. The bulge is of moderate size. No signs of major mergers or significant tidal disturbances are evident, although a possible minor interaction may be present. There does not appear to be a strong central bar.
