This galaxy exhibits a somewhat elongated morphology. The central region presents a smooth appearance with a concentrated, bright core, suggesting an older stellar population. Extending outwards from the core is a fainter disk or arm structure. The color gradient within the galaxy indicates potential variations in stellar populations, with the central regions appearing redder and the outer disk exhibiting bluer hues. There are some potential indications of minor gravitational disturbances or tidal features. The shape of the galaxy appears more cigar like rather than round, but not overtly so. Overall, this galaxy appears to be transitioning from a smooth to more defined morphology.
