The galaxy presents as a relatively smooth, elliptical form. The central bulge exhibits a high surface brightness, with a color profile appearing slightly yellowish, suggesting an older stellar population. Moving outward from the core, the galaxy fades gradually into a less defined halo. The morphology indicates it is likely an early-type galaxy, with little indication of spiral arms or prominent dust lanes. There is very slight evidence of some asymmetry or minor disturbance in the outer regions, but its overall structure is largely undisturbed.
