The galaxy exhibits a complex morphology suggestive of an ongoing or recent merger event. The central region displays a bright, compact core, possibly indicative of an active galactic nucleus or a dense stellar population. The overall light distribution appears relatively smooth, but with noticeable disturbances and asymmetries. There are at least three bright areas that may be separate galaxy cores, each with its own degree of red-shift and distinct color profile.

The galaxy's shape is broadly elliptical but with some deviation that may be due to interaction from the merger. There are suggestions of tidal tails or extended structures emanating from the main body. The overall color of the system is towards the redder end of the spectrum, consistent with an older stellar population and/or significant dust obscuration. The central core has a slightly more pinkish tone suggesting a younger stellar population, which may be associated with a burst of star formation in that area, triggered by the merger event.
