The galaxy presents a largely smooth, elliptical morphology with a central, luminous bulge. There is some faint evidence of a disk-like structure, although this is not well defined. The overall color appears to be somewhat redder with a faint hint of blue. There is no apparent major disturbance or interaction with neighboring galaxies, indicating it is likely a relatively isolated system. The galaxy exhibits an approximately rounded shape, with only a small deviation from circular symmetry. There is no discernible spiral arm structure, further reinforcing the classification as an elliptical or lenticular type. The galaxy has an estimated effective radius of approximately 3 kiloparsecs. The star formation activity is low, with minimal presence of bright, young stars.
