The galaxy appears to be a luminous elliptical galaxy, exhibiting a generally smooth and rounded morphology. There is little evidence of spiral arms or a distinct disk structure. The central bulge is bright and concentrated, decreasing in luminosity towards the outer edges, with a notable lack of pronounced features or irregularities. The galaxy appears to be in a relatively quiescent state, with little ongoing star formation evident from the limited color information available. Some very minor disturbances in the outer regions cannot be ruled out but any potential interaction appears minimal. The overall color profile suggests an older stellar population is dominant. The morphology leans towards being well-rounded, showing it is not particularly elongated.
