The galaxy presents an elongated, elliptical morphology. It exhibits a smooth, featureless structure, lacking prominent spiral arms or a distinct dust lane. The central region displays a higher surface brightness, suggesting a concentration of stars toward the core. The galaxy's color appears generally blue-white, indicative of a population of relatively young, hot stars. The overall impression is that of an early-type galaxy, possibly an elliptical or lenticular galaxy, with ongoing, albeit low-level, star formation. There is some evidence of minor gravitational disturbance within the galaxy.
