The galaxy presents as a fairly regular elliptical morphology, exhibiting a smooth, concentrated central bulge that dominates the overall structure. The light profile appears centrally peaked, with a gradual decrease in brightness moving outward from the core. There are no apparent spiral arms or prominent dust lanes visible, indicating a lack of significant ongoing star formation in a disk-like structure. The galaxy displays a yellowish-orange hue, suggestive of an older stellar population consisting primarily of evolved stars. There is a slight extension of the galaxy along one axis, resulting in a subtle deviation from a perfectly circular shape. No signs of tidal disturbances or interactions with other galaxies are evident. The overall impression is that of a relaxed and relatively undisturbed elliptical galaxy.
