The object presents as an elongated, cigar-shaped galaxy. It appears largely smooth in texture, with no obvious spiral arm structures or prominent dust lanes visible. The color gradient transitions smoothly from a central yellowish-orange core to bluer hues toward the outer regions of the disk. This color variation suggests a possible difference in stellar populations, with older, redder stars concentrated in the center and younger, bluer stars in the periphery. There is a subtle warp or curvature visible along the major axis, potentially indicative of a past or ongoing gravitational interaction, but no clear signs of major disruption or tidal tails are immediately apparent. Overall, the galaxy displays characteristics consistent with an early-type spiral or lenticular galaxy, with relatively low levels of recent star formation.
