The galaxy appears as a centrally concentrated, relatively smooth structure. It has an elongated shape with a somewhat elliptical morphology. The galaxy exhibits a colour gradient, with a more reddish hue towards the central region, potentially indicating an older stellar population. The outer regions of the galaxy appear bluer, suggesting the presence of younger stars or ongoing star formation. There are no obvious signs of strong spiral arm structure or a prominent central bar. The disk of the galaxy appears relatively undisturbed, with only minor indications of tidal features or interactions.
