The galaxy presents as a relatively compact object, exhibiting a somewhat elliptical morphology with a smooth overall appearance. The central region displays a higher concentration of luminosity, transitioning outwards to a more diffuse halo. There is a distinct color gradient; the core exhibits a strong reddish-orange hue, suggestive of an older stellar population, while the outer regions are slightly bluer, hinting at ongoing or recent star formation activity, although the overall star formation rate appears relatively low. There may be some minor disturbances in the outer regions, but overall the galaxy appears relatively isolated. The galaxy is relatively massive.
