The galaxy presents an elongated, cigar-shaped morphology, suggesting it is an edge-on spiral or possibly an elliptical galaxy with significant flattening. The central bulge appears bright and concentrated, exhibiting a yellowish-orange hue, which could indicate an older stellar population. Fainter, bluer light extends from the central bulge into the disk, which is harder to see due to its edge-on presentation. There is a hint of possible dust lane absorption along the galaxy's major axis, though the image resolution limits definitive confirmation. The outer regions of the galaxy are diffuse and less defined. There are no visible distinct spiral arm structures. Given its overall smooth appearance, it is likely in a relatively quiescent state, with a comparatively low star formation rate.
