The galaxy presents as a flattened, elongated structure. A distinct color gradient is observed across the galactic body, transitioning from a warmer, reddish hue on one side to a cooler, bluer tint towards the opposing end. The redder end may indicate an older stellar population. The overall morphology suggests that it could be an edge-on spiral galaxy, but the image quality and lack of distinct spiral arm features mean a definitive classification is difficult. It may also possibly be a lenticular galaxy.

The overall shape is significantly elongated, with a cigar-like profile, indicating non-sphericity. The structure appears relatively undisturbed with a low chance of a major merger or significant tidal interactions. The galaxy is of intermediate size, not extremely large nor extremely small. Overall, the galaxy appears to be a relatively smooth structure.
