The galaxy presents a generally smooth, elliptical morphology with a high degree of roundness. Its core exhibits a bright, concentrated luminosity, transitioning gradually to a fainter halo. The color appears to be predominantly yellow-red, suggesting an older stellar population. There is no evidence of spiral arm structure or significant dust lanes. A possible minor asymmetry or disturbance is visible, hinting at a potential past or ongoing interaction. The galaxy's spatial extent suggests it is a fairly massive object.
