The galaxy appears as a faint, elongated structure with a noticeable central bulge. It exhibits a flattened, disk-like morphology, but the resolution is insufficient to resolve distinct spiral arms. There's a slight indication of asymmetry in the overall shape, possibly suggestive of tidal interactions or recent minor mergers, although no strong tidal tails are observed in the available image. The color distribution is relatively uniform across the galaxy, with a subtle reddening towards the central bulge compared to the outer regions of the disk, potentially indicating an older stellar population in the nucleus and ongoing star formation in the disk. The galaxy's size appears moderate, and it is relatively isolated within the observed field.
