This galaxy presents as a spiral, with a noticeable central bulge. The spiral arms are tightly wound and somewhat fragmented, exhibiting a bluish hue indicative of younger stellar populations and active star formation. The core appears yellowish-white suggesting a concentration of older stars. The galaxy exhibits a moderate inclination with an estimated size of 10 kpc. There may be signs of a faint bar structure within the central region, along with moderate disturbances. There is no indication of interaction with any other galaxies.
