The galaxy presents as a relatively smooth, elliptical structure with a high Sersic index, suggestive of a bulge-dominated morphology. It exhibits a yellowish-white hue, indicating a population of older stars and a reduced presence of active star formation. The overall shape appears slightly elongated, with an ellipticity of approximately 0.7. No obvious spiral arms or dust lanes are discernible. The galaxy's radial light profile demonstrates a concentrated central region that gradually diminishes outwards, confirming that it is bulge-dominated. Based on the faintness in FUV and NUV magnitudes, this galaxy does not appear to be undergoing substantial star formation, which is also confirmed by the redder color, a larger u-r color index than typically seen in star forming galaxies.