The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high surface brightness with a yellowish-white hue, indicating a potential concentration of older stellar populations. Fainter, reddish tones are asymmetrically distributed in a small section of the galaxy, potentially indicating regions of on-going or recent star formation. There is no apparent spiral structure or bar visible. The overall morphology suggests a galaxy in a state of relatively low activity, with a moderately high mass, and a redshift that places it at a considerable distance. It appears largely undisturbed, exhibiting no obvious signs of a major merger event, although the slight asymmetry may indicate a minor interaction.
