The galaxy presents a smooth, elongated morphology. It exhibits a predominantly blue hue, suggesting ongoing or recent star formation activity. The light is concentrated in the center of the galaxy, with a less concentrated diffuse halo that extends in a cigar-like shape. There are no readily apparent spiral arms or a distinct disk structure. There are suggestions of minor disturbances within the galaxy, but no large, extended structures that would obviously indicate ongoing mergers. Based on the color and morphology, the galaxy appears to be relatively quiescent with a low rate of star formation.
