This galaxy appears to be a relatively massive early-type system, potentially a lenticular or elliptical galaxy, exhibiting a smooth and centrally concentrated morphology. The light profile suggests a significant spheroidal component. There is a suggestion of a disk-like structure. The overall colour is redder than many galaxies, indicating an older stellar population and lower levels of current star formation activity. There is no noticeable strong dust lane or prominent spiral arm. The apparent roundness suggests that the galaxy is viewed close to face-on or is intrinsically close to spheroidal. There may be signs of minor disturbance or interaction with nearby companions, however this is not obvious. The colours are consistent with its distance. 
