The galaxy presents as a relatively faint, elongated object. Its shape is significantly more extended in one dimension, suggesting an edge-on or highly inclined disk morphology. There is a smooth, concentrated central bulge that gradually fades into a less defined disk. The disk exhibits a subtle color gradient, with a slightly bluer tint visible along the edges of the galaxy, possibly indicating regions of more active star formation within the spiral arms, although distinct arm structures are not clearly resolved. Overall, the galaxy appears to be in a relatively isolated environment, with no obvious signs of major mergers or tidal interactions with other galaxies.
