The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a spheroidal morphology, appearing mostly round in projection. There is evidence of a faint disk structure or minor disturbances, but the dominant feature is its smooth, elliptical-like shape. The central bulge of the galaxy is prominent, suggesting an older stellar population. The galaxy appears to be undergoing low levels of star formation activity. There is no major merger apparent, but there are subtle distortions in its morphology which could be attributed to a previous minor interaction. The overall color suggests a mix of stellar populations, with the bulge potentially redder than the outer regions.
