The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The light distribution appears relatively uniform, lacking prominent spiral arms or distinct features. The core exhibits a yellowish hue, possibly indicating an older stellar population. A faint, diffuse halo or envelope appears to extend outwards from the central region. There is little evidence of ongoing star formation within the galaxy based on the color profile and the smooth overall appearance, though low levels are expected based on the data. The general shape is roughly round. Possible minor disturbance is not evident.