The galaxy appears as a lenticular or early spiral type, with a prominent bulge and a relatively smooth disk. The central bulge exhibits a yellowish-white hue, suggesting a population of older stars. The disk surrounding the bulge shows a bluer tint, hinting at ongoing or recent star formation. The galaxy displays an elongated shape, appearing cigar-shaped, indicating a significant axis ratio. There's no obvious evidence of strong tidal features or major disturbances, though there is some minor asymmetry and disturbance in the outer disk regions. Overall, it seems to be a relatively isolated galaxy undergoing moderate star formation in its disk.
