The galaxy presents as a centrally concentrated object, exhibiting a smooth and relatively featureless morphology. Its overall shape appears approximately elliptical, with a moderate degree of roundness. The core region displays a yellowish-orange hue, possibly indicating the presence of an older stellar population. Moving outwards from the core, the color transitions towards a slightly bluer shade, suggesting the presence of some ongoing star formation in the outer regions, but the color is mostly red. There is no strong evidence of spiral arm structures or significant dust lanes. The galaxy appears relatively isolated, with no obvious signs of ongoing or recent mergers or tidal interactions, but some minor disturbances cannot be ruled out. The galaxy exhibits a moderate redshift. Overall, the galaxy appears to be a relatively evolved system, potentially undergoing a moderate level of star formation.
