The object appears as a single, relatively compact galaxy with an estimated effective radius of approximately 1.5 arcseconds. The galaxy's morphology is somewhat ambiguous, exhibiting features that could be interpreted as either a smooth elliptical or a disk galaxy with significant disturbances. The light profile displays a bright, concentrated core, surrounded by a more diffuse, extended halo.

The color indices suggest the presence of both young and old stellar populations. The inner core is notably brighter than the outer regions. There are morphological indications of potential tidal interactions or past mergers, characterized by minor asymmetries or disturbances in the galaxy's structure. 
