The galaxy presents as a spiral type, observed at an oblique angle. Its central bulge is prominent and exhibits a yellowish-orange hue, indicative of an older stellar population. Faint spiral arms extend from the central bulge. The arms display a bluer tint, suggesting the presence of younger, hotter stars and ongoing star formation. The disk appears somewhat disturbed, potentially indicating a past or ongoing minor interaction with another galaxy. The galaxy appears of medium size, and exhibits a moderate amount of star formation.
