The galaxy presents a largely smooth and rounded morphology, exhibiting characteristics of an early-type galaxy. It has a concentrated central region with a gradual decline in brightness towards its outer edges. There is no discernable spiral structure or prominent dust lanes. The galaxy appears relatively isolated, with no obvious signs of tidal disturbances or ongoing merger activity. The overall color is slightly redder, suggesting an older stellar population with a relatively low rate of on-going star formation. It measures approximately 5.7 kpc across.
