The galaxy exhibits a distinct spiral structure, with clearly discernible spiral arms extending from a central bulge. The spiral arms appear somewhat loosely wound, suggesting a flocculent or intermediate spiral type. The galaxy displays a bar feature, as evidenced by a slightly elongated central region. The bulge is moderately sized, and the overall disk appears relatively face-on. The galaxy shows indications of possible minor disturbances in its structure, perhaps resulting from minor interactions or internal processes. There is no strong evidence of major merging activity or significant tidal distortions. The color distribution across the galaxy suggests a mix of stellar populations, with a yellow-ish central bulge potentially indicating older, redder stars, and bluer regions within the spiral arms possibly indicative of ongoing star formation.
