The galaxy presents a relatively smooth, elliptical morphology. Its core exhibits a high degree of radial symmetry, and there are no distinct spiral arms or bar structures visible. The light distribution appears concentrated towards the center, indicative of an older stellar population. The galaxy exhibits a yellowish color, consistent with a population of evolved stars with lower rates of current star formation. There's no indication of significant dust lanes or recent merger activity. There might be a faint, extended halo surrounding the central region, but the signal is weak. The galaxy appears as an isolated system.
