The galaxy presents as a somewhat amorphous structure, exhibiting characteristics of both a smooth elliptical galaxy and a more complex spiral or irregular type. There is a central concentration of light, appearing yellowish in color, suggesting an older stellar population. The outer regions show bluer hues, hinting at some ongoing star formation, albeit potentially at a low rate. Evidence suggests it is neither perfectly smooth nor displaying a clear spiral structure; it features some irregular patches. The galaxy does not appear to be strongly edge-on. Some minor disturbances in its morphology suggest a possible past interaction or minor merger event, although there is no strong evidence of a major ongoing merger.
