The galaxy presents as an elongated, disk-like structure viewed nearly edge-on. A prominent central bulge is observed, exhibiting a rounded morphology and an apparent concentration of older stellar populations indicated by its yellowish-orange color. The disk component of the galaxy appears relatively smooth, with no readily discernible spiral arm structure. There may be some blue regions associated with potential star formation, as seen as a light blue tint. The absence of significant tidal features or morphological disturbances suggests that the galaxy is not currently undergoing a major merger event, but there may be a minor interaction with the blue region.
