The galaxy presents as an elliptical or lenticular system, exhibiting a smooth, diffuse light distribution with no apparent spiral arm structure. The galaxy's morphology is elongated, with a cigar-like shape. A distinct color gradient is observed, shifting from a reddish hue toward the core to a greenish-blue tint in the outer regions, potentially indicating varied stellar populations, dust content, or differing rates of star formation across the galactic disk. No significant signs of tidal disruption or interaction with other galaxies are visibly evident, with no apparent major disturbances or merging activity, suggesting a gravitationally stable system.
