The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears to be predominantly elliptical, exhibiting a high degree of circularity. There is a discernible, though not prominent, disk-like structure surrounding the central bulge. The galaxy appears to be fairly isolated. There does not appear to be signs of substantial tidal disruption or interaction with other galaxies. There might be slight internal disturbance, but not a major collision. The color profile indicates the presence of an older stellar population.
