This galaxy exhibits an elongated, disk-like morphology, suggesting it is likely a spiral or lenticular galaxy viewed edge-on or at a high inclination. The central region appears brighter and more concentrated, possibly indicating the presence of a bulge. There's a color gradient across the galaxy; the central bulge appears more yellowish-orange, possibly indicating an older stellar population. The outer regions of the galaxy have bluer tints, which could imply the presence of ongoing star formation. There's a distinct dust lane visible as a dark band bisecting the galaxy, obscuring some of the light. The galaxy appears relatively smooth in structure, but there may be faint hints of spiral arms or other features. The overall shape is oval, with axis ratio of ~ 0.6.