The galaxy presents as a relatively smooth, disk-shaped structure. The central bulge exhibits a pronounced, elliptical morphology with a yellowish hue, suggestive of an older stellar population. Surrounding the bulge is a flattened disk, displaying a greenish-blue tint that may indicate the presence of younger, hotter stars and regions of active star formation. There are hints of subtle disturbances in the outer regions of the disk, potentially indicating past or ongoing minor interaction with another galaxy. The galaxy appears largely isolated, with no obvious signs of a major merger or tidal disruptions. Its overall form suggests a classification as a late-type spiral galaxy or a lenticular galaxy transitioning from a spiral morphology due to a low star formation rate.
