The galaxy appears to be a relatively smooth, elliptical-type galaxy with a concentrated central bulge. It is not perfectly spherical, exhibiting a slight elongation. The galaxy displays a prominent, bright core region with a gradual decrease in luminosity towards its outer edges. There is no apparent spiral arm structure or distinct dust lanes visible within the galaxy's disk. The object's overall color suggests a mix of stellar populations, with the central region appearing slightly bluer than the surrounding halo. There is no evidence of ongoing major merger activity or significant tidal disturbances impacting the galaxy's structure. The object exhibits characteristics consistent with a moderate level of star formation.
