The galaxy appears as a relatively smooth, centrally concentrated object. Its overall morphology suggests an elliptical type, lacking prominent spiral arms or a distinct disk structure. The light distribution is largely uniform, exhibiting a radial decrease in brightness from the core outwards. Color gradients are subtle, though the central region seems slightly yellower compared to the outer regions, possibly indicating an older stellar population. There is no obvious evidence of ongoing major mergers or significant tidal disturbances, and the galaxy appears fairly isolated. There are no prominent dust lanes or regions of intense star formation visible. The galaxy's shape appears close to circular.
