The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits a subtle elongation, deviating slightly from a perfectly circular morphology. The color gradient suggests a possible aging stellar population, with a yellowish core. The outer regions display a hint of bluer hues. There is no strong evidence of spiral arm structure or significant dust lanes. There may be a faint, low surface brightness disk or extended halo surrounding the central bulge. Indications from citizen scientist data suggest that this galaxy has a fairly high probability of being a smooth galaxy rather than one with prominent features or disk. It also does not appear to be undergoing a major merger or experiencing significant disturbances.
