The galaxy presents as a centrally concentrated, largely featureless object. It exhibits a generally smooth, elliptical morphology with a high degree of circularity. The galaxy's light profile is relatively uniform, lacking prominent spiral arms, bars, or other distinct features typically associated with disk galaxies. There is a suggestion of a color gradient, with the core appearing slightly more yellow, possibly indicating an older stellar population towards the center, with bluer, therefore younger, populations on the outer edges. The overall colour of the galaxy is tending towards the redder end of the spectrum suggesting the galaxy is old with ongoing, but slow, star formation. There is no evidence of tidal tails, strong dust lanes, or merging activity within the limits of image resolution and depth.
