The galaxy presents a generally smooth morphology, with a high degree of central concentration. It appears nearly circular in shape, showing minimal deviation from roundness. There is no discernible spiral structure or prominent disk features. The light profile suggests a bulge-dominated system with a centrally peaked luminosity. The galaxy's color is generally consistent with an elliptical classification. There is a subtle color gradient from the center to the outer regions of the galaxy, with the center being yellower in color. There is no strong evidence of recent or ongoing major merger events. The faintness of the system suggests it is an intermediate mass system. Star formation is likely very low, if at all present.
