The galaxy presents as an elliptical morphology, appearing largely smooth and spheroidal. It has a subtle, elongated shape. The light is brightest near the center, with the light gradually diminishing towards the edges. It appears to be a relatively low-mass galaxy, with a moderate star formation rate, given the slightly blue hue. There are no visible signs of active galactic nuclei or significant dust lanes. There is no evidence of recent or ongoing major mergers or tidal disturbances. It looks like a rather isolated system with a tranquil evolutionary history.
