The galaxy presents a generally smooth and elliptical morphology, with a high degree of central concentration. There is a distinct color gradient, shifting from a more yellow-white core to a bluer outer region. No prominent spiral arms or bar structures are discernible. The galaxy appears to be relatively undisturbed, without any major signs of ongoing mergers or tidal interactions. Its shape is more in between round and cigar-shaped, but leaning more towards round. The outer regions appear diffuse, fading gradually into the background sky, suggesting a lack of sharp edges or truncation in its stellar distribution. Star formation is relatively low compared to the galaxy's mass.
