The galaxy presents a generally smooth, elliptical morphology. The light profile appears centrally concentrated with a bright, yellowish core indicative of an older stellar population. There is a gradual fall-off in luminosity with increasing radius, transitioning to a bluer hue in the outer regions, hinting at the presence of some younger stars and possible ongoing, but low-level, star formation. Faint wisps or irregularities might be present, possibly indicative of minor gravitational interactions or disturbances in the past. The overall shape tends toward round, exhibiting some deviation from a perfect sphere.
