This galaxy presents as a highly inclined, possibly edge-on, disk galaxy. The disk exhibits a noticeable dust lane bisecting its length, obscuring a portion of the starlight. The light distribution indicates a centrally concentrated bulge, though it appears relatively small and not overly prominent. The galaxy displays a gradient in color along its length, transitioning from slightly more yellow-orange hues in the bulge region to a bluer tint in the outer disk. This color gradient likely suggests regions of ongoing star formation within the disk, while the central bulge contains an older stellar population. There may be some minor tidal disturbances or interactions with a close neighboring galaxy. Its disk does not appear perfectly flat and even, hinting at some gravitational interactions. The galaxy's overall structure is relatively undisturbed, maintaining a fairly organized and symmetric form. The current star formation rate seems to be relatively low. The mass of the galaxy is estimated to be moderate.
