The galaxy presents a generally smooth morphology, with a high degree of central concentration. The light distribution appears largely spheroidal, suggesting a classification as an elliptical galaxy or a lenticular galaxy seen face-on. There is no obvious spiral structure or a well-defined disk. The object exhibits a color gradient, transitioning from a more yellow hue towards the center to a slightly redder color in the outer regions. The galaxy appears to be relatively undisturbed, lacking any signs of major mergers or tidal interactions. There may be some minor disturbance in the outer regions. Its round morphology indicates little rotation. Overall, the galaxy gives the appearance of an evolved stellar population and a relatively low rate of current star formation.
