The galaxy presents a generally smooth, elliptical morphology. Its light is concentrated towards the center, with a gradual decrease in brightness extending outward, approximately 4 kiloparsecs in radius. The core exhibits a yellowish-white hue, suggesting an older stellar population dominates the central region. There is an absence of distinct spiral arms or prominent dust lanes. The outer regions appear fainter, with a subtle color gradient toward redder tones, potentially indicating a diminishing population of younger, bluer stars further from the galactic nucleus. The galaxy does not appear to be undergoing any major merging events or showing significant tidal disturbances. The morphology is consistent with a quiescent galaxy, possibly with a low rate of ongoing star formation.
