The galaxy presents a generally smooth appearance, suggestive of an elliptical morphology or a lenticular-type disk galaxy observed face-on. The primary light emission is concentrated in a central, bright region, potentially indicative of an active galactic nucleus (AGN) or a dense stellar population within the galactic core. Some visual evidence suggests a slight disturbance to the overall smoothness, a minor asymmetric structure potentially related to a recent or ongoing interaction. The dominant color is yellowish, which hints at an older stellar population, and/or substantial dust obscuration. There is evidence for some activity with its star formation, but low compared to other galaxies.
