The galaxy presents a generally smooth morphology, with a high degree of central concentration. It appears elliptical in shape, with a relatively high degree of roundness. There is a color gradient present, with the core exhibiting a yellowish-white hue and the outer regions appearing more reddish. This may indicate an older stellar population concentrated towards the galactic center, with younger, bluer stars in the outer regions. The galaxy does not show any obvious signs of tidal disturbances or ongoing major mergers, but the redness of the outer regions may indicate a relatively small amount of star formation. There are no obvious spiral arm structures or a prominent disk. Overall, the galaxy appears to be a relatively undisturbed system, likely an elliptical galaxy that may be undergoing modest star formation.
