The galaxy presents as a relatively smooth, centrally concentrated object with a primarily yellow-orange hue in the central region, suggesting an older stellar population. It exhibits a moderate degree of roundness in its overall morphology. There is a slight suggestion of disk-like structure, but the galaxy appears largely spheroidal. No strong evidence of spiral arms or significant dust lanes is discernible. Faint bluish regions are noted in the periphery, which may indicate regions of more recent, but subdued, star formation. There is no obvious indication of significant tidal features or ongoing major mergers, though some minor disturbance cannot be ruled out.
