The galaxy presents as a moderately luminous, disk-shaped system with an estimated radius of approximately 5.7 kpc. The structure exhibits characteristics of an early-type spiral or a lenticular galaxy, showing a distinct central bulge that dominates the overall light distribution. The bulge exhibits a smooth texture and a yellowish color, suggestive of an older stellar population. Fainter spiral arms or a disk component are present, extending outward from the bulge; however, these features are not sharply defined. A slight bluish hue is apparent in the outer regions, which may indicate areas of modest star formation. No major disturbances or signs of a significant merger event are obvious; however, minor asymmetrical features may hint at past interactions.
