The galaxy presents as a fairly smooth, centrally concentrated object. Its overall morphology suggests an elliptical or lenticular classification, with no obvious spiral arm structures visible in this image. The light distribution is brightest in the core, fading gradually towards the outer edges. The core exhibits a yellow hue. The galaxy is moderately bright, indicating a substantial stellar population. It appears relatively isolated, with no immediately obvious signs of major interactions or mergers with other galaxies. Subtle irregularities are visible, suggesting some mild disturbances in the recent past. The overall shape is more "in between" than either round or cigar shaped, suggesting a fairly normal or typical morphology. The overall color profile indicates a significant population of older stars, consistent with a relatively low rate of star formation.
