The galaxy presents as a centrally concentrated spheroid with a smooth, diffuse light distribution.  It exhibits a color gradient, appearing bluer toward the center and subtly redder in the outer regions. The overall shape is elongated, with a cigar-like appearance. There is no visible evidence of spiral arms or a distinct disk structure.  No significant dust lanes or prominent star-forming regions are discernible.  The galaxy appears relatively isolated, with no obvious signs of tidal interactions or major disturbances in its morphology, however a small disturbance cannot be ruled out. The general appearance suggests an evolved system with ongoing, albeit relatively low, star formation.
