The galaxy presents as a relatively smooth, elliptical-like structure with a noticeable elongation. The light distribution appears centrally concentrated, fading gradually towards the outer edges. There's a subtle color gradient visible; the central region appears slightly yellower, potentially indicating an older stellar population, while the outer regions show hints of bluer hues, suggesting the presence of younger, hotter stars, though this is not prominent. The galaxy's overall morphology lacks distinct features such as spiral arms or a prominent disk. There is no obvious sign of strong tidal disturbances or recent major merger events. The galaxy appears relatively isolated, showing no clear signs of interaction with other nearby galaxies.
