The galaxy presents as a relatively face-on spiral galaxy, although it is slightly inclined. The central bulge is quite prominent and appears yellow-orange, suggesting an older stellar population. Fainter spiral arms extend outward from the central bulge, displaying a bluer hue indicative of ongoing star formation. These arms appear somewhat tightly wound, hinting at a flocculent structure. There is some evidence of a possible bar structure bisecting the central bulge. While the overall structure appears relatively undisturbed, there might be some minor irregularities present, which could be indicative of a past or ongoing interaction. The light distribution suggests the presence of dust lanes within the spiral arms, though this is difficult to discern. The galaxy appears relatively isolated.
