The galaxy presents as a generally smooth, elliptical-like structure. Its overall color profile appears relatively red and yellow-shifted, suggesting an older stellar population. The galaxy's central bulge is notably bright, indicating a concentration of stars or potentially an active galactic nucleus. Some evidence suggests a possible minor disturbance in the galaxy’s morphology, perhaps due to a small interaction or tidal effect on its outer regions, though this could also be attributed to imaging noise. The shape appears mostly round, with a slight elongation, but is not highly asymmetric or disturbed. There is a weak indication of ongoing star formation. Overall, the galaxy appears as a fairly massive system, in the range of around 10^10 solar masses.
