The galaxy presents as a generally smooth and elliptical object, with a length-to-width ratio suggesting an elongated, cigar-like morphology. The central region exhibits a concentrated luminosity, appearing bright and yellowish, indicating a likely concentration of older stellar populations. Moving outwards from the core, the luminosity gradually decreases. The outer regions display a slightly bluer hue, which may indicate the presence of some younger stars, albeit in smaller quantities compared to the central bulge. There is no obvious evidence of spiral arms or a well-defined disk structure. The galaxy appears relatively undisturbed, with no major distortions or signs of ongoing mergers.
