The galaxy presents as a slightly elongated or cigar-shaped object. A bright central region, potentially indicative of a galactic bulge or active galactic nucleus, dominates the galaxy's core. Extending outward from this central region are fainter, diffuse regions of light. These outer regions exhibit a somewhat mottled or disturbed appearance. There is evidence of asymmetry in the distribution of light. The blue hue in the outer regions may suggest younger stellar populations and ongoing star formation. Overall, the galaxy appears to be undergoing some level of disturbance, potentially due to interaction with another galaxy or recent merger event.
