The galaxy appears as a centrally concentrated, bright elliptical with a smooth morphology. The core exhibits a yellow-white hue, potentially indicating an older stellar population with fewer ongoing star formation activities. There is a slight elongation to the galaxy's shape, deviating from a perfectly circular profile. A faint, diffuse halo surrounds the central region, extending outwards and gradually fading into the background. There is no significant evidence of spiral arms or prominent dust lanes. Overall, the galaxy's structure suggests a relatively evolved system, likely nearing the end of its star-forming lifecycle. There is a very slight disturbance on the left side of the galaxy.
