The galaxy appears as a relatively bright, centrally concentrated object. Its overall morphology is smooth and elliptical in shape, with no discernible spiral arms or bar structure. The galaxy exhibits a yellowish-red hue, suggesting an older stellar population with less ongoing star formation. There is no apparent dust lane or significant irregularities in its form. The galaxy shows high degree of roundness, with very little asymmetry or elongation. There's no indication of strong tidal interactions or mergers, with no obvious companion galaxies or disturbed features. The light is generally smooth, indicating that it is primarily a collection of older stars.