The galaxy presents as an elliptical-like system, exhibiting a centrally concentrated bulge with a relatively smooth light distribution. The overall shape is elongated, with an ellipticity suggesting a flattened spheroidal structure. Faint, diffuse extensions are tentatively observed along the major axis, possibly indicating tidal features or a disrupted morphology resulting from past interactions. There is a color gradient visible, with the central region appearing slightly redder compared to the bluer hues observed in the outer regions. This difference in color suggests varying stellar populations, with older, redder stars likely dominating the core and younger, bluer stars contributing to the outer disk. There is a faint hint of a disk and dust lane present. Given the red shift, this galaxy appears to be at a considerable distance. 