The galaxy appears to be a spiral, presented at a slight angle to our line of sight. The disk component shows a delicate structure, with regions of active star formation traced by a bluer hue, primarily observed in the outer arms. There are spiral arms, with a medium winding. The central bulge is not particularly prominent, with the light appearing to be somewhat evenly distributed between the bulge and disk, but with a slight concentration in the center. There is a potential, albeit small, interaction or minor disturbance visible that could potentially be the signs of a past merger. The galaxy exhibits a mix of colors, with the central regions appearing more yellow-white, indicative of an older stellar population, while the outer arms show bluer concentrations. 
