The galaxy presents an overall smooth morphology, appearing as a flattened spheroid. The central region exhibits a brighter, more concentrated light profile, suggestive of a prominent bulge. Moving outwards from the center, the light intensity gradually diminishes, transitioning into a fainter, more diffuse disk component. The disk's shape is somewhere between round and cigar-shaped, and it shows a slight tilt relative to our line of sight. There's no obvious signs of spiral arms or significant dust lanes within the galaxy's structure. There are minor disturbances that are slightly present within the galaxy. There are no signs of major galaxy mergers or strong tidal distortions. Overall, the galaxy shows a rather smooth, evolved appearance.
