The galaxy presents as a moderately bright object with a generally smooth, centrally concentrated morphology. It appears relatively compact with a diffuse, extended halo. The color gradient indicates a dominant older stellar population in the central region. The overall shape is elliptical or nearly round. No obvious spiral arm structures or significant dust lanes are discernible at this resolution. There are slight indications of minor irregularities in the outer regions, but the overall structure is generally undisturbed. Based on its color and morphology, it is likely undergoing moderate star formation. The light is shifted towards the red end of the spectrum, which means this galaxy is relatively far away. Overall the galaxy has intermediate mass, based on its size and luminosity.
