The galaxy presents as an elliptical morphology, exhibiting a smooth, largely featureless structure. It appears highly concentrated with a bright, well-defined core that diffuses outwards into a less dense halo. The overall color is dominated by redder wavelengths, suggesting an older stellar population and low ongoing star formation. There is no clear evidence of spiral arms or a prominent disk. The light distribution is fairly symmetrical, indicating a relaxed system without major disturbances or ongoing merger activity. A slight elongation is observed but it is not cigar shaped.
