The galaxy presents as a relatively smooth, elliptical morphology. The central region exhibits a high surface brightness and a yellowish hue, likely indicating an older stellar population. The outer regions gradually decrease in surface brightness, transitioning to a bluer color, potentially signifying ongoing star formation. There is a slight elongation of the galaxy's shape, though it is generally rounded. No signs of major mergers or significant tidal disturbances are apparent, although some minor irregularities can be detected that may be the sign of a minor disturbance or a nascent spiral arm structure, although it cannot be definitively identified. The galaxy's overall color profile suggests a moderate redshift, with the intrinsic blue light from younger stars being shifted towards the red end of the spectrum.
