The galaxy presents as a spiral galaxy with a prominent central bulge. The bulge exhibits a yellowish hue, suggestive of an older stellar population. Spiral arms are visible, though somewhat tightly wound. Two primary arms are discernable, emanating from the central bulge. The disk appears relatively smooth, although some patchy regions of bluer light are present in the spiral arms, hinting at regions of ongoing star formation. The galaxy is oriented at a slight incline relative to our line of sight. There is no obvious evidence of strong tidal interactions or a recent merger event. A subtle bar feature may be present, bisecting the central bulge. The overall color suggests a galaxy with intermediate star-formation activity.
