The galaxy exhibits a largely smooth morphology, with a primarily elliptical or spheroidal appearance. The overall shape is somewhat rounded, with minimal visual distortion suggesting any ongoing major merger activity. A small disk component may be present, but it is poorly defined. The light profile suggests a centralized concentration of older stellar populations, with a redder color index in the central regions that likely contain a higher proportion of evolved stars. The galaxy is of intermediate mass, and exhibits a low to moderate star formation rate. The specific star formation rate is particularly low, indicating that star formation is relatively quiescent compared to the galaxy's stellar mass. The colour of the light being emitted suggests that the galaxy is at a considerable distance.
