The galaxy presents as a centrally concentrated, elliptical-like object with a smooth, diffuse appearance. The core exhibits a bright, yellowish hue, suggesting an older stellar population dominating the central region. Moving outwards from the core, the light gradually fades into a more reddish, less defined region with some hints of more diffuse edges. There is no significant evidence of spiral arm structures or a prominent disk. The overall shape appears roughly circular, with a slight suggestion of elongation, though the resolution limits a more detailed morphological classification. There is no noticeable ongoing major merger activity or significant tidal distortions of its shape.
