The galaxy presents as a bright, disk-shaped system viewed at an angle of approximately 17 degrees from face-on. The central bulge is prominent and appears spheroidal, exhibiting a yellowish hue suggestive of an older stellar population. A distinct bar feature is present within the galaxy's central region, characterized by a concentration of luminosity extending horizontally. The surrounding disk exhibits a more mottled appearance with some indication of spiral arm structure, although these are poorly defined. The overall color of the disk appears somewhat bluer than the bulge, potentially indicating the presence of younger, hotter stars within the spiral arms. There is some indication of a faint, extended halo surrounding the main galactic body. The galaxy's shape is moderately elliptical.
