The galaxy appears to be a relatively smooth, elliptical or lenticular type, showing little evidence of spiral arms or significant dust lanes. Its overall shape is somewhat elongated, displaying a moderate ellipticity rather than being perfectly spherical. The galaxy's light profile appears centrally concentrated, fading gradually towards its outer edges. No distinct nucleus is discernible within the resolution of this image. The color seems consistent with an older stellar population, with a bias towards redder wavelengths, suggesting a lack of ongoing, significant star formation activity. There is no obvious indication of a recent major merger event or strong tidal disturbances, though a possible minor interaction or disturbance cannot be entirely ruled out at this resolution.
