The galaxy presents a generally smooth and centrally concentrated morphology. It exhibits an elliptical shape, with a noticeable elongation but is mostly "in between". The light profile appears to gradually fade from a bright, somewhat unresolved core to a diffuse outer envelope. There is no prominent spiral arm structure or obvious dust lane obscuration visible. Based on color indices, the galaxy likely hosts an older stellar population with moderate star formation. There are no signs of major disturbances, but the possibility of minor interaction cannot be ruled out based on its morphology alone. The estimated size of the galaxy is around 5 kpc.
