The observed galaxy presents a complex morphology, suggestive of an ongoing or recent merger event. The central region displays a somewhat amorphous structure with no distinct nucleus. Multiple luminous knots or condensations are apparent within the central area and throughout the extended halo, possibly indicative of active star-forming regions triggered by the interaction.

The overall shape departs from a smooth elliptical form, exhibiting irregularities and extended tidal features. Evidence of disturbed galactic structure is apparent in the form of faint, diffuse extensions emanating from the central region. The light distribution appears relatively smooth, with variations in intensity but no distinct spiral arm structure. Based on the observed features, the galaxy is likely undergoing a significant gravitational interaction, altering its original morphology.
