The galaxy presents a generally smooth, elliptical morphology. The light distribution indicates a centrally concentrated spheroid, with a major axis that is discernibly longer than its minor axis, giving it a somewhat cigar-shaped appearance. It appears to be dominated by an older stellar population, evidenced by the yellow-red hue of its central regions.  There is a suggestion of bluer, potentially younger stars or star-forming regions in the surrounding regions. There is no indication of a prominent disk component, tightly wound spiral arms, or significant tidal disturbances. The overall structure suggests a relatively undisturbed system.
