The galaxy presents as a spiral type, viewed at a relatively face-on orientation. It exhibits a notable central bulge that appears moderately prominent and bright. The surrounding disk is visibly structured, featuring spiral arms that wind somewhat tightly around the bulge. Two of these arms are fairly distinct.  There may be evidence of a weak bar feature extending through the central bulge. The galaxy appears relatively isolated, with no obvious signs of major interaction or merging, although some minor disturbances could be present. The system shows signs of ongoing star formation within the spiral arms, but the color suggests overall it may be in the green valley.
