The galaxy appears to be an elliptical galaxy, exhibiting a smooth, largely featureless morphology. It has a generally round appearance in the image. There is a slight color gradient, transitioning from a slightly bluer hue in the center to a somewhat redder periphery. This suggests the possibility of a radial distribution of stellar populations, with younger, hotter stars concentrated in the core and older, cooler stars more prevalent in the outer regions. There is no evidence of spiral arms, a bar, or other distinct disk-like structures. No clear signs of ongoing major mergers or significant tidal disturbances are apparent; however, the central region shows a possible slight irregularity in its surface brightness profile, which may indicate past minor interactions.
