The galaxy appears to be a relatively compact, elliptical system. The core region displays a concentrated brightness, with a smooth, gradual falloff in luminosity towards the outer edges. The color profile suggests a higher concentration of older stellar populations, indicated by its yellowish-orange hue. There is little evidence of prominent spiral arms or significant dust lanes. The overall morphology indicates a system that is likely not undergoing major mergers or significant star formation at the present epoch, as the galaxy has a fairly amorphous structure. Faint, diffuse light extends outwards from the central region, suggesting a smooth halo, with no signs of strong tidal disturbances or interactions.
