The galaxy presents as a relatively compact, luminous structure. Its morphology appears to be transitioning, exhibiting characteristics of both smooth and possibly disturbed systems. There is a central concentration of light, a yellowish hue in the center suggests an older stellar population dominates the core. Fainter, bluer regions surround the core, hinting at ongoing star formation. There is the possiblity of a tidal feature or minor interacting galaxy, indicative of past or ongoing gravitational interactions. The primary structure has a shape between a perfect circle and that of a cigar. Evidence suggests that the merger is not at the final stage, as there are a small number of major disturbances within the morphology.
