The galaxy presents as a somewhat elliptical object, exhibiting a centrally concentrated luminosity profile. The core region is notably brighter, shifting toward yellower wavelengths. Moving outwards from the core, the color transitions towards a redder hue, which is indicative of older stellar populations and possibly dust attenuation. The object displays a relatively smooth texture, with minimal discernible structural features such as spiral arms or prominent dust lanes. A high degree of central concentration and smooth profile are consistent with an early-type galaxy morphology. There is a subtle suggestion of disturbance on the periphery, but these may also be issues with image quality. Overall, the galaxy appears to be a relatively mature system, potentially undergoing a minor merging event.
