The galaxy appears to be a lenticular or early-type spiral galaxy, with a smooth, centrally concentrated bulge and a faint, diffuse disk. The bulge exhibits a yellowish-white color, suggestive of an older stellar population. There is some evidence of a disk component extending from the bulge, it shows a more bluish tint, potentially indicating the presence of younger stars and ongoing star formation. The galaxy is elongated and ellipsoidal in shape and exhibits a smooth profile, with no obvious signs of spiral arms or distinct morphological features. There are no signs of major disturbances, tidal tails, or other indicators of a recent merger event.
