The galaxy presents as an elliptical structure with a noticeable central bulge. The bulge appears to be the brightest region, characterized by a yellowish-orange hue, suggesting an older stellar population. A flattened disk surrounds the bulge, oriented edge-on relative to our line of sight. The disk exhibits a bluer tint. Dust lanes appear to be present, although partially obscured. There may be some faint spiral structure visible in the disk, but further observation would be required to verify this. The overall structure displays a relatively smooth profile. The outer regions of the galaxy gradually fade into the background.
