The galaxy presents as a moderately bright, elliptical-shaped object. Its core region exhibits a high surface brightness, appearing almost uniformly luminous and bright. Proceeding outwards from the center, a gradual decrease in luminosity occurs with increasing radius, and we can discern the inner halo region. A subtle blue tinge is observed throughout the galaxy, potentially indicating ongoing star formation or the presence of a relatively young stellar population. The galaxy's overall structure appears smooth and relatively undisturbed; there is no apparent evidence of significant tidal interactions or major merger events. There is no apparent disk structure and no defined spiral arms.
