The galaxy presents a relatively smooth, elliptical morphology. There is little evidence of strong spiral arm structure or significant star formation regions from visual inspection of the image. The light distribution appears centrally concentrated, with a gradual decrease in intensity outwards, consistent with an early-type galaxy. The galaxy exhibits a fairly homogenous color profile, with the core being a bright yellow and slowly fading to a red/orange halo. There is no distinct nucleus. The absence of major disturbances or mergers indicates a dynamically relaxed system. The estimated size of the galaxy appears relatively small compared to other galaxies.
