The galaxy presents a generally smooth and elliptical morphology. Its light profile appears largely uniform, with a concentrated central region. The galaxy exhibits a yellowish hue, indicating a population of older stars and a reduced rate of recent star formation. There is no obvious spiral arm structure or significant dust lane obscuration visible in the image. The overall appearance suggests a galaxy that is relatively evolved and quiescent. A slight asymmetry in the outer regions of the galaxy hints at a possible minor interaction or recent accretion event. 
