The galaxy presents as a relatively smooth, elliptical-like structure. It appears highly concentrated, with a bright, well-defined core that gradually fades into the surrounding halo. The color gradient suggests an older stellar population, possibly dominated by redder stars. There is little to no evidence of spiral arms or significant dust lanes; the overall morphology indicates minimal recent major merging activity or internal disturbances. The galaxy shows a near-spherical distribution of light, though a slight ellipticity can be perceived. No signs of tidal tails or other interaction remnants are observable.
