The galaxy presents as a smooth, elliptical form, with a high degree of central concentration. Its color profile suggests an older stellar population, with a yellowish-red hue dominating the central bulge. The isophotes appear largely regular, with no immediately obvious signs of strong tidal features or major disturbances. The minor disturbances present are likely due to a small amount of star formation occurring, however, it appears to be at a slow pace. A slight elongation is discernible, moving from the upper left to lower right, but the overall shape is far from cigar-like. The galaxy appears relatively isolated, with no clear evidence of a recent or ongoing major merger event.
