The galaxy presents a mostly smooth morphology, with a concentrated central bulge that appears to be composed of older stellar populations, indicated by its yellow-orange hue. Fainter, bluer colors are visible in what could be considered the disk; there appears to be some presence of on-going or recent star formation. The overall structure seems to lean towards an elliptical, though there are faint indications of a potential spiral structure if the disk is indeed present. There seems to be some minor disturbance in the galaxy's morphology, possibly indicating a minor merger or tidal interaction event.
