The galaxy presents as a spiral structure, exhibiting prominent, well-defined spiral arms emanating from a central bulge. The spiral arms appear somewhat flocculent, with segments displaying a medium degree of winding. Two major spiral arms seem to be present. The central bulge appears moderately bright. There is a possible bar feature, with a moderately defined structure visible. The disk is not perfectly face-on; it shows a slight inclination. The overall light distribution appears to be relatively smooth, with some texture in the spiral arms, possibly indicating star-forming regions. There is no significant evidence of a major merger or tidal disturbances in the main body of the galaxy. There appears to be blue stars, indicating recent star formation. The galaxy's shape is elongated, with the major axis longer than the minor axis.
