The galaxy exhibits a generally elliptical morphology, elongated along its major axis. A smooth, centrally concentrated bulge is apparent, transitioning into a fainter, more diffuse halo. The bulge displays a yellowish-white color, suggesting an older stellar population. Some features include faint spiral arms, indicated by subtle variations in the blue hue along the galaxy's disk and some minor signs of disruption along the edges. The galaxy has a notable inclination, with the disk appearing tilted relative to the observer's line of sight. A visual inspection indicates that the galaxy is of intermediate size and mass. The overall color is dominated by older stars, which suggests a low star formation rate. The presence of some blue regions suggests some ongoing, but limited star formation.
