The galaxy presents as a highly inclined, likely edge-on, disk galaxy. There is a distinct central bulge that appears luminous. While the resolution is limited, a subtle boxy shape is hinted at within the bulge, though a more rounded structure appears more prominent. The overall impression of the disk is smooth and lacking in distinct spiral arm features, which are obscured due to the edge-on orientation. The galaxy exhibits color gradients, with a brighter, potentially younger stellar population implied by a bluer hue in the disk region. No signs of major mergers or significant tidal disturbances are visible, indicating a relatively isolated evolutionary path.
