The galaxy presents an elliptical morphology with a notable central bulge. The core exhibits a reddish-yellow hue, suggesting a population of older stars, likely a result of decreased recent star formation activity within the galactic nucleus. Moving outward from the core, the galactic disk displays a bluer color, indicative of ongoing or recent star formation involving younger, hotter stars. There appears to be a slight asymmetry or disturbance in the outer regions of the disk, possibly the result of a minor gravitational interaction with another galaxy or a past merger event. The galaxy's smooth overall appearance suggests a relatively evolved system, yet the bluer regions indicate that star formation is still actively occurring, albeit at a moderate rate.
