This galaxy presents as a relatively smooth, elliptical-like structure. Its color profile suggests an evolved stellar population, as the light appears redder than galaxies with active star formation. There is a strong central bulge with a high degree of symmetry. A faint disk component may be present, but it is not well-defined. There is a possibility of a minor tidal interaction or disturbance, indicated by a slight asymmetry in the isophotes or a subtle extension of the galaxy's halo. Given the overall morphology and color, the galaxy is likely a massive system with a significant number of stars. Evidence indicates suppressed star formation within the galaxy. The possibility of a merging event seems reasonable given the disturbance present in the galaxy.
