The galaxy presents an overall asymmetrical morphology. The central region exhibits a bright, diffuse glow with a slight elongation, suggesting a possible bar or distorted core. Patches of bluer light are seen interspersed throughout the galaxy, indicating regions of potential star formation. The presence of some regions of redder light may indicate older stellar populations and/or dust obscuration. There are possible signs of gravitational disturbance, with a faint arc-like structure that may indicate a tidal feature or a past merging event. Some irregularities exist and no spiral arms are apparent.
