The galaxy presents as a spiral type, viewed at a slight angle relative to face-on. The central bulge appears prominent and concentrated, exhibiting a yellowish hue indicative of an older stellar population. Fainter spiral arms are visible extending outwards from the bulge. They appear tightly wound, with a somewhat patchy and discontinuous structure. The arms display a bluer color, suggesting the presence of younger, hotter stars and regions of active star formation. The overall morphology suggests that this is a well-formed spiral galaxy, showing no obvious signs of major disturbances or ongoing mergers.
