The galaxy presents as a moderately luminous object, with a distinctly elongated, cigar-shaped morphology. Its color profile indicates a predominantly older stellar population, evidenced by the reddish-yellow hue which dominates the galaxy's light. The central bulge is prominent, exhibiting a high degree of smoothness. There are subtle signs of possible features or a disk component. The overall appearance suggests a system that is either actively undergoing or recently completed a phase of significant quenching of its star formation. The lack of strong blue colors further supports the interpretation of low ongoing star formation. While the primary body of the galaxy appears undisturbed, there are faint indications of minor tidal disturbances, potentially indicating past interactions with smaller companion galaxies.
