The galaxy presents as a complex system, potentially undergoing an interaction or merger event. There are two primary luminous components visible. One appears to be a somewhat elliptical, concentrated central bulge, exhibiting a yellowish hue indicating an older stellar population. The second, a disk-like structure, is visibly tilted relative to our line of sight. This disk shows some hint of spiral arm structure, although it is not well defined. 

The overall color suggests moderate star formation activity, potentially concentrated in the disk, with relatively little ongoing star formation in the bulge. A separate, compact, and bright object is located close to the galaxy.

Based on the morphology, there is evidence of tidal features or distortions, suggesting a possible interaction with a nearby galaxy or a previous merger event. The overall structure is somewhat disturbed, supporting the hypothesis of ongoing or recent gravitational interaction.
