This galaxy exhibits a disturbed morphology, suggesting a possible interaction or merger event. The light distribution appears somewhat asymmetric, with two discernible concentrations of light that could be interpreted as galactic nuclei or high stellar density regions. The overall color profile indicates the presence of both older stellar populations, inferred from the redder hues, and possibly younger, star-forming regions indicated by some bluer tinges, though the color balance is predominantly skewed toward older stars. There is an apparent elongation or tidal feature extending from one of the light concentrations, further supporting the hypothesis of gravitational disturbance. No defined spiral arms or clear disk structure are visible. The galaxy has a relatively smooth overall appearance but appears to be in an active state of evolution.
