The galaxy presents as a somewhat elongated, lenticular structure. Its central bulge is prominent and appears relatively smooth, suggesting an older stellar population. The disk component is faintly visible, exhibiting a subtle blue hue indicating the presence of some younger stars. The overall color profile suggests that star formation is present but subdued. The morphology is indicative of a relatively evolved system that has largely exhausted its gas supply, leading to a decline in star-forming activity. The shape seems more cigar shaped, with no major distortions.
