The galaxy presents a generally smooth, elliptical morphology. The light distribution appears concentrated towards the center, with a gradual decrease in surface brightness towards the outer edges, forming a cigar-like shape. There is a subtle color gradient, with the central region exhibiting a slightly bluer hue than the periphery, suggesting younger stellar populations towards the core. There is no apparent spiral arm structure or significant dust lane obscuration. No major merging or tidal disturbances are apparent. The galaxy does not appear to be particularly active in star formation based on the image.
