The galaxy presents as a disk galaxy, viewed at a high inclination angle. The morphology appears predominantly smooth with a bright, concentrated central bulge, gradually fading outwards into the disk. The disk exhibits a relatively smooth texture with subtle variations in color and brightness suggesting some spiral structure, although not sharply defined. The disk appears elongated, with a ratio of major to minor axis significantly greater than 1, indicating a flattened shape. The galaxy displays a color gradient with a bluer, likely younger stellar population in the outer regions of the disk, transitioning to a redder, likely older stellar population towards the central bulge. No obvious signs of active galactic nuclei or significant starburst activity are immediately apparent from the morphology alone, suggesting a relatively quiescent galaxy. There is no evidence of tidal tails or obvious signs of interaction. The morphology suggests the galaxy is relatively undisturbed.
