The galaxy appears as a moderately sized, relatively smooth, and concentrated structure. Its morphology seems to be primarily elliptical, with a high degree of central concentration and a lack of prominent spiral arm features. The color profile is generally consistent across the galaxy, with a slight shift towards redder hues. This suggests an older stellar population and reduced ongoing star formation. There is no noticeable active galactic nucleus, nor any obvious signs of tidal disturbances or mergers. The overall light distribution is elliptical, tending towards a more rounded shape. There seems to be a slight asymmetry present, with a minor disturbance potentially present, though it could be a visual artifact.
