The galaxy presents as a generally smooth, elliptical morphology. The central region exhibits a high surface brightness, with a yellowish-white coloration suggesting an older stellar population. Moving outwards from the core, the galaxy fades in surface brightness, transitioning to a bluer hue in the outer regions. This subtle color gradient may indicate the presence of some ongoing, low-level star formation in the outer disk. The galaxy's overall shape is moderately elongated. There is no obvious spiral structure or bar visible in the image. There is a slight asymmetry in the outer isophotes, potentially indicating a minor gravitational interaction or disturbance.
