The galaxy appears as a relatively bright, concentrated object. It presents a smooth, somewhat elliptical morphology, and it has a yellow-white hue, possibly indicative of an older stellar population with a smaller fraction of young, blue stars. There is no prominent spiral structure, and the concentration of light towards the center suggests a substantial bulge component. Faint hints of possible tidal disturbances or minor asymmetries are present, suggesting past or ongoing interactions with other galaxies. Overall, this appears to be an early-type galaxy at a considerable distance, exhibiting minimal star formation.
