The galaxy presents as an interacting system of considerable complexity.  The primary body exhibits a generally smooth, elliptical morphology.  The light profile of the galaxy is concentrated centrally and appears more pronounced towards the core. The color is predominantly yellow-orange, suggestive of an older stellar population.

A secondary object, with similar coloration, is observed in close proximity to the primary galaxy. This could indicate a merger event of similar stellar populations. There is visual evidence of tidal disturbances or connections between these two objects.

The overall form is distorted, lacking a well-defined disk structure. Indications of recent or ongoing interactions are apparent. Further investigation is warranted to determine precise dynamics and star formation history.
