The galaxy presents a generally smooth, elliptical morphology. Its shape appears to be somewhere between round and cigar-shaped. The galaxy exhibits a distinct color gradient, with a brighter, bluer core that fades outward into a redder halo. This suggests a possible difference in stellar populations, with younger, hotter stars concentrated in the core and older, cooler stars populating the outer regions. There is no apparent disk structure or spiral arms visible in this image, which suggests that it may be an elliptical galaxy. There are no obvious signs of significant tidal disturbances or mergers with other galaxies. Any recent disturbances would be considered minor, and this galaxy is likely to be isolated.
