The galaxy presents a centrally concentrated morphology, appearing largely smooth in texture. The light profile suggests a dominant bulge component. The central region exhibits a bright, yellow-white hue, indicative of an older stellar population. The outer regions display a fainter and somewhat redder color, suggesting the presence of dust or a population of cooler, older stars. There is a slight elongation observable in the galaxy's shape, although it does not deviate significantly from a circular form. There is potential evidence of a weak or disturbed disk, given its appearance, but the overall morphology remains bulge-dominated. There is potentially minor disturbances near the disk, but without higher resolution imagery, classification of a merger is unclear.
