The galaxy presents as a moderately luminous, elliptical system. The color profile suggests a dominant population of older stars, with a yellowish-orange hue indicative of relatively low star formation. The galaxy displays a smooth, concentrated morphology, lacking prominent spiral arms or distinct features. The apparent shape is somewhat elongated, but largely uniform. There are no visible signs of significant tidal disturbances or ongoing major mergers. The central bulge appears bright and well-defined, suggesting a high concentration of stellar mass towards the galactic nucleus. Faint extended emission is potentially observed around the main galactic body, but is close to the noise level.
