The observed galaxy presents a flattened, elongated morphology, appearing as a cigar shape on the plane of observation. Its light profile shows a smooth, centrally concentrated bulge with a distinct color gradient, transitioning from a yellow-white core to a slightly bluer, fainter outer disk. There is no obvious spiral structure discernible. The smoothness of the light distribution and the lack of prominent dust lanes suggest it is likely an early-type spiral galaxy or a lenticular galaxy, rather than a late-type spiral with active star formation. There are no indications of any major merging events or significant tidal disturbances in this galaxy. The light is dominated by older stellar populations, and there is very little recent star formation activity.
