The galaxy presents a generally smooth appearance, with a centrally concentrated light profile, suggestive of an elliptical morphology. While a definitive disk structure is not readily apparent, there is a slight elongation and some subtle features that suggest it might be more of a lenticular galaxy with a faint disk component. The galaxy's color is relatively uniform across its body, primarily appearing as a yellowish-orange hue. This indicates a population of older stars, potentially with ongoing star formation. There is no clear evidence of strong spiral arms or dust lanes. Some minor disturbances appear to be present, possibly indicating a past interaction. Overall, the galaxy seems to be in a relatively quiescent state, with a likely low rate of star formation.
