The galaxy presents as a centrally concentrated object, exhibiting a generally smooth morphology. The light distribution appears elliptical, with the major axis only slightly more extended than the minor axis, suggesting a low ellipticity. The core region of the galaxy shows a bright, concentrated emission, possibly indicating the presence of an active galactic nucleus or a region of high stellar density. The surrounding halo fades outwards gradually, without any strong evidence of spiral arm structures. Color gradients are subtle, with the central regions exhibiting a yellowish hue, potentially indicating an older stellar population, while the outer regions show slightly bluer tones, which could be a hint of younger stars or lower metallicity gas. There is little visible dust obscuration. No tidal features or signs of recent major merger activity are immediately apparent in this image.
