The galaxy presents a largely smooth, elliptical morphology. It appears relatively round in shape, with no obvious strong spiral arms or bar structures. The color profile is dominated by light with longer wavelengths, suggestive of an older stellar population with lower rates of star formation. There is a hint of some minor disturbance or potential interaction with another nearby object, as indicated by a slight asymmetry or irregularity. This object appears to be relatively massive, as it is quite bright.
