The galaxy presents as an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The core region displays a yellowish hue, suggestive of an older stellar population. Moving outward from the center, the color shifts slightly to a redder tone, implying a potential gradient in stellar age or metallicity. No spiral arm structures or dust lanes are discernible within the image, and no obvious signs of recent or ongoing major merger activity are apparent. Minor disturbances might be present, however, it is difficult to resolve. The galaxy appears relatively isolated, with no obvious companion galaxies in close proximity to induce tidal interactions. Based on the ellipticity, the object appears more "in between" round and cigar shaped, rather than truly circular or highly elongated.
