The galaxy appears to be a relatively smooth, disk-like structure, with a central bulge that exhibits a concentrated brightness. It presents a flattened morphology, trending towards an elliptical shape, but not fully spherical. There is a color gradient noticeable, with the central bulge exhibiting a yellowish hue that suggests an older stellar population. Emanating outward, the disk appears somewhat bluer, potentially indicative of ongoing or recent star formation. 

There appears to be minor disturbances in the galaxy's shape, possibly resulting from a minor interaction or merger event, though no major disturbances are evident.
