The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The color profile appears generally redder, suggesting an older stellar population within the galaxy. There is minimal evidence of spiral arms or dust lanes; the structure seems largely featureless. The galaxy appears moderately bright with a significant spheroidal component. Any visible structure indicates that this galaxy has likely experienced minimal disturbances or interactions with neighboring galaxies. The shape, although generally elliptical, does exhibit a slight deviation from perfect roundness, leaning towards an in-between round shape.
