The galaxy presents a generally smooth, elliptical morphology, with a high degree of central concentration. The light distribution is relatively even and consistent with a spheroid dominated system. There is some suggestion of a slight asymmetry or perturbation in the outer isophotes, possibly indicating a minor interaction or past merger event. The overall color is slightly redder in the central region, potentially indicating an older stellar population. The effective radius appears to be relatively small, suggesting a compact structure. A small region displays a green hue towards the center of the galaxy, which could suggest recent star formation. There is no strong evidence of spiral arms or a well-defined disk structure. 
