The object presents as two distinct, interacting galactic structures. The larger, primary structure appears relatively smooth and elliptical in morphology. Its color gradient suggests an older stellar population, with a predominantly yellowish-orange hue indicating the presence of evolved stars. There is little evidence of spiral arms or prominent dust lanes within the larger structure.

A smaller, secondary object is observed in close proximity to the primary galaxy. This secondary structure exhibits a more irregular shape and similar coloration. The proximity and distorted morphology of both structures suggest an ongoing or recent gravitational interaction, likely a galactic merger. The system, overall, is compact, with no clear evidence of extended tidal tails or significant star formation regions visible in this image. The system appears relatively evolved with a high estimated mass.
