The galaxy presents as a fairly smooth, elliptical-like structure. Its core appears luminous, with a concentrated central region exhibiting a yellow-orange hue, indicative of an older stellar population. The galaxy rapidly fades outwards from the bright center, transitioning into a less intensely colored halo. There is minimal evidence of spiral arms or defined dust lanes. The overall shape of the galaxy is generally round. No signs of any major merging events are observed, with the galaxy exhibiting a largely undisturbed morphology.
