The galaxy presents as a relatively smooth, elliptical object with a notable central bulge. Its color profile suggests a dominance of older stellar populations, exhibiting a yellowish-orange hue that intensifies towards the core. The galaxy appears elongated, deviating significantly from a perfect circular shape. While the overall structure seems undisturbed, a subtle asymmetry might indicate minor tidal interactions or internal activity. There is no clear evidence of spiral arms or prominent dust lanes within the visible structure. The light distribution is concentrated around the central region, with a gradual decline in brightness toward the outer edges, which appears more diffuse.
