The galaxy presents as a smooth, centrally concentrated object, consistent with an elliptical morphology. It exhibits a slight elongation, appearing somewhat cigar-shaped rather than perfectly spherical. There is no discernible spiral structure or prominent dust lanes. The color profile suggests a population of older stars, leaning towards the red end of the spectrum, but also showing evidence of some blue light emission, possibly indicating ongoing, although limited, star formation. There may be a minor gravitational disturbance or interaction occurring, as evidenced by the slight asymmetry in its overall form, though no major merger events are obvious.
