The galaxy presents as a relatively smooth, elliptical-like structure. Its central region displays a concentrated luminosity, appearing a yellowish-orange hue, indicative of an older stellar population. A faint, extended halo surrounds the core, exhibiting a subtle gradient in luminosity as it fades into the background. The overall morphology suggests a system dominated by spheroidal components, showing little to no evidence of prominent spiral arms or a well-defined disk. Based on its color and morphology, the galaxy appears to be in a relatively quiescent state, with a low rate of ongoing star formation. Subtle color variations are observed in the outskirts, hinting at the presence of a small population of younger, bluer stars. There is no visual evidence of strong tidal interactions or recent merger events. The shape appears close to circular.
