The galaxy appears to be a spiral galaxy with a relatively small bulge. The spiral arms seem well-defined with moderate winding. There's evidence of ongoing star formation within the arms, observable through the presence of blue-ish regions. The central bulge exhibits a yellow-ish hue, possibly indicating an older stellar population. There appears to be a slight asymmetry in the distribution of light across the galaxy, which may be from a previous or current interaction with another smaller galaxy.