The galaxy appears to be a relatively compact system. It exhibits a somewhat elongated, cigar-shaped morphology. A significant portion of the galaxy's light is concentrated in a central region, with a smoother appearance. There are hints of potentially disturbed features, possibly indicative of a minor interaction or ongoing merger event. One side shows a reddened hue, which could suggest enhanced star formation or dust obscuration in that particular region. The overall color is bluish, suggesting moderate ongoing star formation.
