The galaxy presents as a relatively compact object, appearing largely smooth in structure. There is a hint of a disc-like structure, but it is not pronounced. A slight elongation is apparent, but it mostly appears rounded. There is evidence of potential interaction or disturbance present, indicated by subtle irregularities in its form. Based on its color, this object appears relatively quiescent, exhibiting colors consistent with a population of older stars, suggesting a lower rate of star formation. There are no strong indications of any recent major merger events, though minor disturbances might be present.
