The galaxy presents as a somewhat elliptical, relatively smooth structure. There's some indication of disk-like features, but they are not very prominent. The primary body exhibits a generally even color distribution suggesting an older stellar population with suppressed recent star formation. There is some evidence of minor disturbances in the galaxy's structure, possibly suggestive of a minor interaction. The galaxy is moderately rounded in appearance with a slight deviation from perfect circularity. Overall, the galaxy does not seem to be undergoing major merging activity or intense star formation.
