The galaxy presents as a slightly inclined spiral galaxy. Two prominent spiral arms emanate from a central bulge, exhibiting a moderate winding pattern. The arms appear relatively tightly wound closer to the bulge, loosening slightly as they extend outwards. The bulge comprises a significant portion of the galaxy's overall luminosity, indicating a substantial population of older stars. The disk exhibits variations in color, with bluer regions tracing the spiral arms, suggesting ongoing star formation. The galaxy appears to have a small bar. There is no indication of any major disturbances or ongoing merger activity, though minor irregularities in the disk may suggest past interactions or internal processes.
