The observed galaxy presents as a spiral structure, with flocculent arms emanating from a central bulge. The bulge appears moderately sized and displays a yellow-orange hue, indicative of an older stellar population. The spiral arms exhibit a bluer coloration, suggesting ongoing star formation activity. There appears to be two prominent spiral arms wrapping around the central bulge. The arms have a medium winding tightness to them and present themselves more as broad and somewhat fuzzy features. Overall, the galaxy is quite large with what looks to be signs of a potential merger occurring with another smaller galaxy nearby. There is a slight distortion that can be seen with the galaxy in addition to some faint light between the two separate masses.
