The galaxy appears to be a relatively smooth, elliptical-like system, with a bright, concentrated central bulge. The light distribution is dominated by this central region, suggesting an older stellar population. The galaxy exhibits a slight elongation, hinting at a possible deviation from a perfectly spherical shape. There's a subtle color gradient visible, with the central region appearing slightly bluer than the outer regions. This may indicate some ongoing, but limited, star formation activity in the core. The overall structure seems relatively undisturbed, showing no obvious signs of major mergers or tidal interactions, although there is some minor asymmetry in its structure.
