The galaxy presents a generally smooth morphology, characterized by a high degree of central concentration. Its shape appears to be in between round and cigar shaped. The color gradient indicates a concentration of older stellar populations towards the galactic center, with a possible hint of bluer, younger stars in the outer regions suggesting ongoing, albeit low-level, star formation. No strong evidence of spiral arms or a distinct disk component is immediately apparent. The galaxy exhibits a minor degree of asymmetry, but there are no indications of major mergers or significant tidal disturbances. The overall appearance suggests a relatively evolved system with a substantial bulge component.
