The galaxy presents as a spiral system, viewed nearly edge-on. A prominent, bright central bulge is visible, displaying a smooth, concentrated light profile. The disk component is clearly discernible, exhibiting a flattened structure extending outwards from the bulge. The spiral arms appear tightly wound and relatively well-defined, exhibiting a blueish hue, suggestive of ongoing star formation. There is no apparent evidence of a strong bar structure bisecting the bulge region. The outer regions of the disk appear relatively smooth, showing no prominent signs of major tidal disturbances or ongoing mergers, although some minor disturbances are possible. The size of the bulge appears small to moderate in relation to the disk. The galaxy exhibits a substantial disk component, characterized by a moderately high degree of spiral arm presence. Overall, the galaxy appears to be a relatively undisturbed spiral galaxy, likely exhibiting moderate star formation activity.
