The galaxy presents a largely smooth and centralized light distribution, suggesting a morphology leaning towards elliptical or lenticular. The central region appears significantly brighter and more concentrated than the outer regions, with a gradual decrease in luminosity towards the edges. A slight flattening is observed, hinting at a disk-like structure, although it is not prominently defined. The galaxy exhibits a reddish hue, indicative of an older stellar population and relatively little ongoing star formation. There is an indication of some minor disturbances or asymmetrical features, possibly signs of past or ongoing interactions with other galaxies. Overall, the galaxy appears as a mature system, with a well-established structure and limited recent star formation activity.
