The galaxy appears as an elongated, disk-shaped structure with a dominant central bulge. The color profile suggests a relatively evolved stellar population, with reddish hues concentrated toward the central regions and along the main axis of the disk. There is a lack of distinct spiral arm structure, indicating it is likely a late-type spiral or lenticular galaxy. The galaxy appears fairly smooth, with no obvious signs of major ongoing mergers or significant tidal disturbances, although there may be a hint of minor irregularities in the disk. The galaxy is significantly inclined from our line of sight. The overall morphology appears relatively undisturbed.
