This galaxy presents as a relatively compact object. Its overall morphology appears largely smooth, with a possible faint disk-like component oriented horizontally across the image. The galaxy's shape is neither perfectly round nor highly elongated, but rather intermediate. There is a color gradient, transitioning from a yellow-white core to a redder outer region. Evidence for significant ongoing mergers or major tidal disturbances is minimal. Faint structural asymmetries or minor disturbances might be present, but the overall impression is that of a galaxy undisturbed from its quiescent state. Based on the color profile, the inner region may be composed of older, more evenly distributed stellar populations, with a potential for some obscured dust.
