The galaxy presents as an elliptical morphology, appearing largely smooth and featureless. It exhibits an elongated shape, suggesting an 'in-between' to 'cigar' shaped form. The central region displays a concentrated, yellowish-orange hue, indicative of an older stellar population. The outer regions fade into a more diffuse, bluish tint, potentially indicating regions of more recent, though perhaps minimal, star formation. There is no apparent evidence of significant merging activity or major disturbances within the galaxy's structure.
