The galaxy exhibits a prominent central bulge, appearing smooth and bright, which suggests a high concentration of older stars. Surrounding the bulge is a flattened disk component. There is faint, blue-ish structure in the outer regions of the disk, possibly indicative of ongoing star formation. The galaxy appears largely undisturbed, showing only a slight asymmetry. The general morphology leans towards an early-type spiral or lenticular galaxy. Overall, the object is a moderately luminous galaxy with a relatively low star formation rate.
