The galaxy presents a largely smooth, elliptical morphology. Its overall color profile appears to be skewed towards the redder end of the spectrum. The galaxy exhibits a high degree of central concentration with a gradual falloff in surface brightness towards its periphery. No prominent spiral arms or disk-like features are discernible. There is no evidence of active galactic nuclei activity based on the apparent lack of a bright, point-like source in the core. The galaxy does not exhibit any major tidal disturbances or morphological signs of ongoing or recent major mergers. There may be a slight indication of a minor interaction or disturbance in the outer regions. The shape is mostly round.
