The galaxy presents a generally smooth and somewhat elliptical morphology, suggesting a classification along the lines of an early-type spiral or a lenticular galaxy. There's a subtle disk-like component, hinted at by a slightly elongated shape, but without prominent spiral arms.

The color profile appears relatively uniform across the galaxy, with a slightly bluer hue in the central region and more red-ish/yellow in the peripheral regions. The redder colors in the outer regions is indicative of an older stellar population, and the bluer colors in the inner regions are indicative of ongoing or recent star formation.

There is a hint of mild gravitational disturbance, with the overall shape being a little asymmetrical, but no obvious signs of a major ongoing merger. These disturbances point to a possibility of minor interactions with smaller satellite galaxies in the past.
