The galaxy presents a generally smooth, elliptical morphology with a bright, concentrated central bulge. It exhibits a subtle disk-like structure, although the overall shape is not perfectly circular; it shows a slight elongation, verging toward a cigar shape. The primary color is a yellow-orange hue, indicative of a population of older stars. The galaxy appears relatively isolated, with no obvious signs of major interaction or merging events. There may be a very minor disturbance in the outer regions, but the core seems undisturbed. The color distribution suggests a lack of significant ongoing star formation within the main body of the galaxy.
