The galaxy presents as a somewhat smooth, elliptical structure with a concentrated central bulge. The light distribution appears diffused, with a general decrease in intensity from the core outwards. There is a slight elongation, giving it an "in between" roundedness, but it lacks a clear disk-like appearance. Faint features suggest some disturbances. It does not appear to be undergoing a major merger, but there could be minor gravitational disturbances. The color profile indicates it's composed of older stellar populations.
