The galaxy appears as a flattened, elongated disk structure with a noticeable central bulge. It presents a reddish-orange hue, possibly indicative of an older stellar population or significant dust obscuration. The galaxy's disk exhibits some subtle, irregular features rather than a perfectly smooth structure, with hints of possible spiral arm structures. There is a noticeable color gradient across the galaxy, with the central region appearing slightly brighter and more reddish compared to the edges of the disk. Overall, the galaxy appears relatively undisturbed, showing no signs of significant ongoing merger activity or strong tidal interactions. The disk appears to be oriented at a steep angle relative to our line of sight.
