The galaxy presents an elongated, cigar-shaped morphology. It appears relatively smooth in structure with a concentrated central bulge that transitions to a more diffuse, extended halo. The color gradient suggests a possible variation in stellar populations. The core appears yellowish-red, possibly indicating older stars, dust obscuration, or a combination of both. The outer regions fade to a pale yellow, which could indicate a population of younger stars or a change in the dust content within those regions. There is no indication of any major disturbances or ongoing merger events. Based on this and its color, it could be in a transition state between a spiral and elliptical galaxy.
