The galaxy presents a somewhat amorphous structure, appearing neither purely elliptical nor a well-defined spiral. It exhibits a central concentration of light, indicative of a nucleus or bulge, surrounded by a less concentrated halo. This central region shows a slightly reddish hue. Extending outwards from the main body are what appear to be tidal tails or disrupted arms, suggesting an interaction or merger event. These extensions are bluer in color, potentially indicating regions of active star formation. The overall shape of the galaxy is elongated, deviating from perfect sphericity, possibly due to ongoing gravitational disturbances. There are no distinct dust lanes visible. The galaxy is relatively compact and shows signs of moderate star formation.
