The galaxy presents a distinct spiral morphology, with moderately defined spiral arms emanating from a central bulge. The bulge appears significant in size, contributing a substantial fraction to the overall luminosity of the galaxy. While the image resolution is limited, there is evidence of some structure within the arms, possibly indicating areas of active star formation. The arms themselves are not tightly wound, suggesting a less compact spiral structure. No apparent bar feature is visible. The color gradients suggest a transition from older stellar populations in the central bulge to younger, bluer populations within the spiral arms. There is no visually obvious evidence of a major ongoing merger event or significant tidal distortions, but some minor asymmetry within the spiral arms could imply past interaction or disturbance. The disk appears to be oriented close to face-on.