The galaxy presents a generally smooth and elliptical morphology. It exhibits a concentrated, bright central region which gradually diffuses outwards. The color profile suggests a dominant population of older stars, contributing to a yellowish-red hue within the galaxy's core and inner regions. There is no clear evidence of spiral arms or significant dust lanes; the overall structure appears largely homogenous. The shape is close to circular but has a slight ellipticity. There is no apparent interaction with other galaxies or indications of recent major merger events. Overall, the galaxy is likely a massive quiescent galaxy with low current star formation.
