The galaxy presents as a moderately luminous, cigar-shaped system. The central region exhibits a high degree of concentration, with a smooth, elliptical profile that gradually fades into the surrounding galactic halo. A subtle color gradient is observed, transitioning from a yellowish core to a slightly redder outer region. There is no distinct spiral arm structure or prominent dust lanes visible. Overall, the morphology suggests an evolved system, potentially an elliptical or lenticular galaxy, lacking significant ongoing star formation activity. There appears to be no major disturbances or merging events currently in progress, based on its relatively undisturbed, symmetrical structure.
