The galaxy appears to be an elliptical galaxy, displaying a smooth, diffuse morphology without discernible spiral arms or a distinct disk structure. It has an elongated, cigar-like shape, suggesting a significant degree of ellipticity. The galaxy exhibits a color gradient, with a yellowish core and a more reddish, fainter outer halo. This color variation could indicate differences in stellar populations and age, with the core potentially hosting older, redder stars and the outer regions containing younger, bluer stars. No signs of ongoing major merging events or significant tidal disturbances are observed.
