The galaxy presents a largely elliptical morphology with a concentrated central bulge. The light distribution appears smooth and centrally concentrated with no apparent spiral arm structure or distinct features indicating ongoing major mergers. The galaxy exhibits a radial color gradient, appearing yellower or redder towards the center, and bluer towards the outer regions of the galaxy, suggesting a mix of stellar populations, potentially with older stars dominating the central bulge and a younger population existing at the outer edges of the galaxy. There is a subtle deviation from a perfectly elliptical shape with the hint of a disk. There is no significant disturbance in shape or light distribution implying an ongoing merger or tidal interaction. The general appearance is that of a quiescent system with low levels of recent star formation activity relative to its mass.
