The galaxy presents as a disk-shaped system viewed nearly edge-on. A central bulge, characterized by a yellowish hue, is apparent. The disk component exhibits a flattened profile, with evidence of some obscuration, possibly due to dust lanes, though the resolution limits precise identification. The overall color suggests a mixed stellar population, with the central bulge likely dominated by older, redder stars, while the disk shows a bluer component, possibly indicative of ongoing star formation. The galaxy lacks any obvious signs of spiral arm structure or strong tidal interactions. The outer edges of the disk appear diffuse.
