The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits a nearly circular morphology. There's minimal evidence of spiral arm structure or significant dust lanes, although the light is slightly uneven in its distribution. The galaxy displays a gradual color gradient, appearing bluer in the central regions and redder towards the outskirts, which would indicate a difference in stellar populations. The overall appearance suggests that this is a relatively evolved galaxy. I can detect very slight disturbances on the edges of the galaxy, so perhaps there was a minor merger a long time ago, or perhaps it is still accreting smaller galaxies.
