The galaxy presents as a somewhat elliptical structure, with a concentrated central bulge that graduates outward into a fainter, less defined disk. The central region appears yellowish-white, suggesting a population of older stars. Moving outward from the center, a bluer hue becomes more apparent in the disk, indicating the presence of younger stars. While difficult to discern, there are hints of some minor disturbances in the outer regions, though no strong evidence of a major merger event is readily apparent. The overall smooth appearance suggests a classification towards the earlier side of the Hubble sequence.
