The galaxy presents as a slightly elongated or cigar-shaped morphology. A central bulge is readily apparent, appearing brighter and more concentrated than the surrounding galactic disc. The color of the bulge appears more reddish-orange, possibly indicative of an older stellar population.

The outer regions of the galaxy display a flatter, disc-like structure, although it lacks well-defined spiral arms. There is evidence of bluer regions within the disc, suggesting some ongoing star formation, yet it appears quiescent overall. There are no clear signs of a major merger or significant tidal disruption. Some minor disturbances in the outer regions cannot be ruled out, although they are subtle.
