This galaxy presents a moderately inclined disk morphology. The central region appears to exhibit a relatively smooth and concentrated bulge, displaying a yellowish-orange hue suggestive of an older stellar population. Moving outward from the center, the disk shows a subtle transition to bluer colors, especially towards the edges, which hints at the presence of ongoing star formation. There is a possible disturbance or slight asymmetry in the disk, indicating a possible minor interaction or merging event with a less massive object, although the features are not prominent. The dust lanes are not readily apparent, as seen through the bluer patches along the edges.
