The galaxy presents as a slightly elongated, disk-like structure. Its overall color appears reddish, potentially indicating an older stellar population. While a clear bulge is not distinctly visible, the central region exhibits a slightly higher concentration of light compared to the outer disk, suggesting the possible presence of a small central bulge. The disk appears relatively smooth, lacking prominent spiral arm structures, though some subtle variations in brightness are present. There are indications of minor disturbances in the galaxy's form, but it does not seem to be undergoing a major merger event. The galaxy is relatively isolated, with no obvious close companions. The size of the galaxy appears intermediate when compared to other objects in the field of view.
