The galaxy presents as a spiral type, exhibiting a flattened disk-like structure. Prominent spiral arms are visible, suggesting active star formation regions within the disk, seen as areas of bluer light. The central bulge appears moderately sized and exhibits a yellowish color, indicative of an older stellar population. The overall shape appears somewhat elliptical rather than perfectly circular, with a bar-like feature possibly present across the central region, though its structure is not distinctly pronounced. There is no clear indication of any major ongoing merger or strong tidal disturbance. Dust lanes may be subtly interwoven within the spiral arms, obscuring some of the background light. The disk is not perfectly edge on, but rather at an oblique angle.
