The galaxy presents as a spiral type, exhibiting a notable disk structure. A central bulge is visible, appearing somewhat compact and luminous. Spiral arms are clearly defined, winding moderately outwards from the central bulge. The winding of these arms appear tight. Dust lanes appear to be present within the spiral arms, contributing to a somewhat mottled appearance. The galaxy appears relatively isolated, with no immediately apparent signs of major mergers or significant tidal disturbances. There appears to be a bar structure within the central region of the galaxy. The color of the galaxy suggests a mix of stellar populations, with bluer regions within the spiral arms indicative of ongoing star formation.
