The galaxy presents as a smooth, disk-like structure with a prominent bulge. The bulge appears bright and concentrated, exhibiting a yellowish hue, suggestive of an older stellar population. The disk surrounding the bulge is fainter and appears slightly bluer in color, indicating the presence of some younger stars. The galaxy exhibits a slight elongation, appearing more elliptical than circular. No spiral arm structures or significant dust lanes are clearly visible. There is no obvious sign of interaction or major disturbances in its morphology, with the overall appearance indicating a relatively undisturbed system.
