The galaxy presents as an elongated, relatively faint object. Its morphology suggests a disk galaxy viewed at a significant inclination. There is a subtle brightening along what appears to be the central axis, potentially indicating a bulge or a higher density of stars and gas along the galactic plane. The overall color of the galaxy appears slightly blueish, which may indicate ongoing star formation. The disk's edges appear somewhat diffuse, possibly suggesting the presence of dust or a more extended stellar halo. There is no clear spiral structure visible, which could be due to the inclination, dust obscuration, or the intrinsic nature of the galaxy. The lack of significant distortions or tidal features implies that it is likely not undergoing a major merger, however there may be small tidal features present. Based on the apparent size, it seems to be a relatively small and potentially low-mass galaxy.
