The galaxy presents an elliptical morphology, exhibiting a smooth and concentrated light profile. Its shape is neither perfectly spherical nor highly elongated, appearing somewhat in between. There's a discernible central bulge that dominates the galaxy's structure, with a gradual decrease in luminosity towards the outer regions. The overall color suggests a relatively older stellar population, with a greater abundance of redder stars. There may be the presence of a faint disk around the central bulge. There is no evidence of a major merger or significant tidal disturbances from neighboring galaxies, though a minor disturbance can't be ruled out. Star formation appears to be minimal. The galaxy is relatively compact, and its apparent size suggests it is a galaxy at a considerable distance.
