The galaxy presents as a lenticular, disk-shaped structure with a clearly defined central bulge. It exhibits a smooth, symmetrical morphology with a high degree of ellipticity suggesting an edge-on or nearly edge-on orientation relative to our line of sight. The central bulge appears luminous, with light that tends towards yellow, consistent with an older stellar population. Proceeding outwards from the bulge, the disk exhibits fainter, bluer light, implying the presence of younger stars within the disk. The galaxy shows no obvious signs of spiral arm structures or active star formation regions within the visible spectrum, instead it appears quite passive. There appears to be no significant tidal disturbances or signs of ongoing merger activity. Overall, this galaxy appears to be a relatively evolved system with ongoing, but low, star formation.
