The galaxy presents as a relatively smooth, centrally concentrated object, with a noticeable elliptical morphology. Its color gradient suggests an older stellar population, with a dominant yellowish-orange hue indicating lower levels of ongoing star formation activity. There might be very weak evidence of a faint, diffuse disk-like structure surrounding the central bulge. However, the overall appearance is dominated by the smooth and centrally condensed light distribution, typical of an early-type galaxy. There are no pronounced spiral arms or features indicative of active galactic nuclei or major mergers. The galaxy shows some distortion which could be minor disturbances.
