The galaxy presents as a moderately luminous, disk-shaped object with a noticeable central bulge. Its overall color suggests the presence of both older stellar populations in the bulge, indicated by a yellow-red hue, and younger, bluer stars within the disk. The disk is not particularly well-defined, appearing somewhat smooth and lacking prominent spiral arm structures. There are hints of asymmetrical features or minor disturbances in the disk's outer regions. The galaxy exhibits an elongated shape, being significantly longer than it is wide. There may be ongoing, low-level star formation activity present within this galaxy.
