The galaxy presents a largely smooth, elliptical morphology with minimal discernible substructure. The light profile exhibits a concentrated bulge region, characterized by a yellowish hue, indicative of an older stellar population and reduced recent star formation activity. The galaxy appears to be somewhat elongated along one axis, but the overall shape is closer to round rather than a highly flattened disk. There's no clear evidence of spiral arms, bars, or tidal features suggesting recent or ongoing major merger events. The galaxy has a significant mass and a redshift indicating it is relatively distant. The inferred star formation rate is relatively low, consistent with its observed color and morphology. There are hints of a subtle outer halo of fainter light surrounding the central region.
