The galaxy presents as a relatively smooth, elongated structure. The central bulge is bright and concentrated. The surrounding disk shows a bluer hue, potentially indicating the presence of younger stellar populations and ongoing star formation. There may be faint evidence of a disk component, although the image resolution limits definitive assessment. The galaxy exhibits an intermediate ellipticity, appearing neither perfectly round nor highly elongated. There are subtle asymmetries in the outer regions, hinting at possible past minor interactions. The overall color suggests a relatively low star formation rate.
