This galaxy exhibits a predominantly disk-like structure, although the smoothness fraction suggests it may have some elliptical characteristics as well. It appears to be inclined at a relatively high angle with respect to our line of sight, nearing an edge-on orientation.

There is a subtle blue hue suggesting areas of active star formation, most noticeably on the far left side of the galaxy. The galaxy is primarily composed of an older stellar population, with a weak signature of younger, blue stars scattered throughout. A central bulge is visible, gradually fading into the disk. There is some subtle irregular morphology throughout the disk, which could be indicative of minor disturbances or tidal interactions. Based on these observations, the object presents itself as a moderately sized galaxy with a low rate of star formation.
