The galaxy presents as a somewhat smooth, elliptical-like structure. Its morphology is largely dominated by a bright central bulge, suggesting a high concentration of older stars. The galaxy appears elongated, with a cigar-like shape. There is subtle evidence of a faint disk-like structure surrounding the bulge, but any spiral arms are not visible or poorly defined. The galaxy displays a color gradient, shifting from a yellow/white core to a slightly bluer periphery. This bluer hue towards the outer regions may indicate some ongoing, albeit low, star formation. There are no obvious signs of tidal distortions or interactions, indicating that the galaxy is relatively isolated and undisturbed, displaying minimal signs of any past or ongoing mergers.
