The galaxy appears as a relatively small, faint, and somewhat amorphous structure. It presents an elongated shape, possibly indicating a disk-like morphology viewed at an oblique angle or a prolate spheroid. The galaxy's light is dominated by a bluish hue, with a subtle concentration of brighter light towards the central region, suggesting an older stellar population in the nucleus. Irregularities in the outer regions are visible, which may be a spiral arm structure. There is a lack of prominent dust lanes or distinct features; the galaxy exhibits a smooth, diffuse appearance with no bright HII regions, suggesting that the galaxy is undergoing little to no star formation. The galaxy appears undisturbed without signs of tidal tails or other distortions, suggesting it has not undergone any recent major mergers.
