The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated bulge, indicated by the higher surface brightness in the core region. The galaxy displays a gradual decrease in surface brightness moving outwards from the center, suggesting a lack of distinct spiral arms or features. There might be a very slight elongation, giving it a somewhat in-between or rounded shape. There are no obvious signs of major merger activity or significant tidal disturbances in the image. The color profile suggests a relatively older stellar population, with a higher concentration of redder stars towards the central regions and a hint of younger, bluer stars towards the outer edges. Star formation appears to be low.
