The galaxy presents a generally smooth and rounded morphology, though with subtle features suggesting potential disturbances. A significant portion of the light appears to originate from a central region, exhibiting a yellowish-white hue indicative of older stellar populations. There is a fainter, reddish area suggesting ongoing star formation, or dust extinction. The galaxy is not perfectly circular, showing a slight elongation. The overall structure hints at possible minor interactions or mergers in its past, which may be contributing to the observed features.
