The galaxy presents as a smooth, elliptical-like structure with a dominant central bulge. It appears largely featureless in the available image data, exhibiting a high degree of symmetry with minimal visible substructure. The galaxy is mostly round with some cigar-shaped curvature. The galaxy's color profile suggests a population of older stars, leaning towards redder wavelengths. There is no clear evidence of ongoing major star formation or significant dust lanes. The galaxy does not appear to be undergoing any major merger activity. The object could be an elliptical galaxy at a considerable distance.
