The galaxy presents as a disturbed system, likely undergoing or having recently undergone a merger event. The main body appears asymmetrical and elongated, with a possible central concentration of older stars indicated by the yellowish hue at the apparent core. A faint, diffuse, blue-ish halo surrounds the core, suggesting the presence of a younger stellar population, possibly triggered by the interaction. There are structural distortions in the galaxy, possibly tidal tails or bridges, however, it's difficult to assert this with certainty due to the quality of the data. The overall shape deviates significantly from a standard elliptical or spiral morphology, indicative of a system in transition. The apparent size and moderate brightness suggest it is a moderately luminous galaxy at intermediate redshift.
