The galaxy appears as a centrally concentrated object, displaying a predominantly smooth morphology with a relatively round shape. Its core exhibits a bright, yellowish-white hue, suggesting an older stellar population dominates in this region. Moving outwards from the center, the color subtly shifts towards redder tones, which could be indicative of slightly younger stars or the presence of dust. There is a very faint hint of disk-like structure, though this is not prominently visible. No distinct spiral arms or significant morphological disturbances are apparent. The galaxy seems to be relatively isolated and undisturbed.
