This galaxy appears to be a relatively smooth, disk-shaped galaxy viewed at an oblique angle. There are no apparent spiral arms or a prominent bar structure. It appears mostly uniform in color, with a concentration of light towards the center, suggesting a prominent bulge. The overall light distribution is relatively smooth, indicating that this could be an older galaxy with less active star formation. The elongated shape indicates a moderately inclined disk, and its relatively small angular size suggests that it could be a dwarf galaxy. There are no obvious signs of interaction or major disturbances. The overall impression is of a relatively quiescent, well-established galaxy.
