The galaxy presents as a spiral type, exhibiting well-defined spiral arms emanating from a central bulge. These arms appear tightly wound. The central bulge displays a yellow hue, possibly indicating an older stellar population. Evidence for ongoing star formation is suggested by the presence of blue regions within the spiral arms. The galaxy appears to be relatively isolated with no strong signs of major mergers, but some minor disturbances might be present. There is the appearance of a weak bar structure within the central region. The galaxy displays no dominant bulge size.
