This galaxy presents as a relatively smooth, centrally concentrated object. The light distribution is generally elliptical, appearing nearly round. A bright, yellowish core dominates the galaxy's emission, suggesting a significant population of older stars or an active galactic nucleus. The outer regions exhibit a fainter, bluer hue, potentially indicating ongoing, though likely subdued, star formation. There is no apparent strong spiral structure or significant morphological disturbance. The galaxy appears relatively isolated, with no obvious signs of recent or ongoing merger activity.
