The galaxy presents a somewhat amorphous structure, appearing neither purely elliptical nor a well-defined spiral. Its central region displays a moderate concentration of light, suggesting the presence of a galactic nucleus, though it is not exceptionally bright or distinct. The overall color profile tends toward the redder end of the spectrum. The image indicates a possible interaction or merging event. There seems to be evidence of a potential tidal tail or disrupted arm extending from the main galactic body.
