The galaxy presents as a fairly smooth, centrally concentrated object. Its overall morphology appears elliptical or lenticular. A bulge is prominent, dominating the light profile. There is little to no evidence of spiral arms or significant dust lanes. The colour is generally uniform and trending towards the redder end of the spectrum, indicating an older stellar population with less recent star formation. Its shape is moderately rounded. There's no noticeable interaction with any other galaxy, nor are there any strong tidal features indicative of recent mergers. There may be a slight asymmetry to the light distribution, hinting at a possible past interaction, but more data would be needed to confirm that. Overall, it's consistent with a relatively quiescent galaxy that has largely exhausted its supply of gas for forming new stars.
