The galaxy presents as a relatively bright, centralized object with a slightly elongated morphology. The light distribution appears smooth and concentrated towards the center, suggesting a prominent bulge component. There is a subtle transition in color from the central region, which exhibits a yellow-white hue, to the outer regions which fade to a bluer tint. The overall structure suggests a disk galaxy viewed at an angle, with no obvious spiral arms. The surface brightness of the galaxy fades gradually outwards. The absence of prominent features, such as dust lanes or distinct star-forming regions, suggests it is a relatively evolved galaxy. There is a possibility of slight tidal disturbances but the evidence for this is slim.
