The galaxy exhibits a prominent disk structure with a noticeable central bulge. The disk shows evidence of spiral arm morphology, though not highly defined. A bar-like feature appears to traverse the central region of the galaxy. The bulge appears moderately sized in comparison to the overall disk extent. There may be indications of minor disturbances in the outer disk, though a major merger is unlikely. The galaxy is significantly inclined to our line of sight, though not entirely edge-on. The color profile suggests a mix of stellar populations, with a redder central region indicative of older stars and dust, transitioning to bluer hues in the outer disk, potentially representing younger, star-forming regions. The smoothness of the galaxy is not highly dominant, but rather exhibits disk and some featured fractions.
