The galaxy presents as a relatively bright object with a somewhat amorphous, but generally rounded morphology. It exhibits a yellowish-white hue, indicating a mature stellar population. There is a subtle hint of a disk-like structure or spiral arms, although it is not clearly defined. The galaxy appears moderately concentrated, lacking a prominent central bulge, with the light intensity decreasing smoothly towards the outer edges. Some slight disturbances are visible, hinting at a possible interaction or past merger event, although the overall structure is still largely intact. There are some subtle color variations and textures throughout the galaxy, suggesting complex regions of star formation activity in its history. Overall, this is a sizable galaxy with ongoing or recently quenched star formation, appearing largely undisturbed with potential past signs of minor mergers.
