The galaxy exhibits a generally smooth morphology with a dominant spheroidal component. Its overall shape appears relatively round, with only a slight deviation from perfect circularity. There is some suggestion of a faint disk-like structure, though this is not prominent. No major disturbances or signs of ongoing mergers are evident. The color gradient transitions smoothly from a yellowish core to a bluer outer region, indicating a possible radial variation in stellar populations. The bluer hues in the outer regions suggest the presence of younger, hotter stars, while the yellower core may be indicative of older stellar populations. Overall, this appears to be a relatively quiescent system with moderate star formation.
