The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge, which emits a bright, yellowish-white light. This central region appears nearly spherical, with a gradual decrease in luminosity moving outward. There is a subtle transition into a less luminous, more diffuse halo, where the light fades into the background sky. No distinct spiral arms or disk-like structures are discernible in the image. The overall shape is primarily circular with no major distortions or signs of active merging events immediately obvious. Based on the colour profile, a population of older stars is likely dominant within the central bulge, with possibly some presence of ongoing, albeit relatively low, star formation activity.
