The galaxy presents as a fairly smooth, centralized elliptical system. The light profile shows a concentrated core, with the luminosity decreasing gradually outwards. The core appears slightly yellowish in color, suggesting an older stellar population. The outer regions exhibit a more diffuse, bluish tinge. The overall morphology suggests it is a non-disturbed system, with no evidence of strong tidal interactions or ongoing major mergers. The galaxy appears to be a rather massive system with a moderate amount of star formation. There appears to be a disk-like structure, though it is very faint and difficult to discern.
