The galaxy presents as a spiral type, viewed at a moderate inclination. The central bulge appears prominent, with a yellowish-orange hue, suggesting a population of older stars. Two distinct spiral arms are visible, extending from the central bulge. These arms exhibit a tightly wound structure. Star formation seems to be present within these arms, indicated by the presence of bluer regions. There is no evidence of any major merger events, but the spiral arms are somewhat ill defined indicating possible past disturbances. There also does not appear to be a prominent bar structure in the center of the galaxy.
