The galaxy presents as a merging system or a galaxy undergoing a significant gravitational interaction. The primary body of the galaxy appears elliptical in shape, exhibiting a smooth, featureless morphology with a central concentration of light. There is a pronounced tidal tail or arm extending outwards from the main galactic body, indicating gravitational disruption. Within the central region, distinct clumps of enhanced star formation or regions of increased density are visible. The overall color of the galaxy leans towards the redder end of the spectrum, suggesting a population of older stars and potentially a reduced rate of on-going star formation relative to bluer galaxies. There is evidence of a secondary, smaller galactic component in close proximity, further supporting the classification as an interacting system, that looks to be in a later stage of merging with the primary object. The galaxy appears relatively massive.
