This galaxy presents a relatively smooth and rounded appearance. It exhibits a concentrated central bulge, characterized by a yellowish-orange hue, suggesting an older stellar population. The light distribution appears symmetric, with a noticeable lack of spiral arm structures or prominent dust lanes. The surrounding halo is faint and indistinct, blending gradually into the background. The overall morphology indicates a galaxy that is likely elliptical. There is no evidence of tidal disturbances or ongoing mergers.
