This galaxy exhibits a generally smooth morphology. The light is concentrated towards the center, with an elongated shape, appearing more cigar-shaped than circular. There is evidence of a possible interaction or merger event, indicated by a potential minor disturbance. There is a distinct color gradient across the galaxy, transitioning from bluer hues towards a redder region, suggesting variations in stellar populations or dust distribution. Given the observed color and smooth morphology, a considerable fraction of the stellar population may be older and more evolved. However, the presence of bluer light suggests the presence of younger stars and active star formation in a certain region of the galaxy.
