The galaxy presents a roughly elliptical morphology with a smooth, diffuse appearance. The central region exhibits a high degree of luminosity, with a concentration of light suggesting the presence of a galactic nucleus. The light emitted from the central region seems to be more blue in the spectra. There is a smooth transition outwards from the center to the outer edges of the galaxy, with a gradual decrease in surface brightness. The galaxy's overall shape is largely spheroidal. There also appears to be signs of disturbance in the galaxy shape and/or small interactions with another galaxy, particularly on the outer parts of the galaxy. This suggests that the galaxy could be in the process of merging with another galaxy.
