The galaxy presents as a spiral type, with visible arm structures originating from a bright central bulge. The spiral arms are somewhat loosely wound and patchy, suggesting ongoing star formation. A disruption is visible on one side of the galaxy, appearing as a plume or tail extending outwards, suggestive of gravitational interaction or recent merger activity. The central bulge is of moderate size, with a concentration of light in the center. The overall color of the galaxy indicates a mix of stellar populations, with bluer regions likely corresponding to younger, hotter stars within the arms, and a more yellow/white hue in the central bulge implying older stellar populations. There is no obvious bar structure detected. The disk is oriented somewhat face-on, allowing for a view of the spiral features.
