The galaxy appears to be an elliptical type, exhibiting a smooth, relatively featureless morphology. Its overall color profile suggests a redder, and therefore older, stellar population, with a concentration of light towards the galactic center. The galaxy is moderately luminous, with a shape that appears to be somewhere between round and cigar-shaped. There is no clear evidence of a spiral arm structure or significant dust lanes. Close inspection reveals a faint reddish structure beside the galaxy. This could be a result of a minor disturbance, or perhaps a faint tidal tail. However, the main galaxy shows no strong signs of an ongoing major merger or significant interaction with other galaxies.
