The galaxy presents as a diffuse, elongated object with a noticeable color gradient. It exhibits a primarily blue hue throughout the bulk of its structure, suggestive of ongoing or recent star formation. The central region appears somewhat brighter and potentially more concentrated, though still relatively ill-defined. The morphology is disk-like but lacks a clear spiral structure; the apparent elongation could indicate either an edge-on or highly inclined disk orientation. There is also a feature above and to the left of the disk with a more yellow hue, suggestive of older stars and little star formation. Faint features and disturbances are observed that may indicate minor gravitational interaction with another galaxy or an internal perturbation. Overall, the galaxy appears relatively low in mass with a correspondingly low star formation rate.
