The galaxy presents an overall shape that is neither purely elliptical nor a well-defined spiral. There is a central bulge, and some evidence of disturbed features. The primary component is a relatively smooth, bright central region appearing slightly elongated. Extending from this core are fainter, more diffuse structures. These regions suggest possible tidal features or disrupted arms resulting from gravitational interactions, potentially indicative of a merging system. There is a hint of an irregular disk component but it is difficult to ascertain. The colors across the galaxy appear mixed, with a central blue-white region and hints of redder areas possibly associated with older stellar populations or dust lanes, giving a complex overall color profile. It shows signs of considerable recent star formation.
