The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits a nearly circular morphology with a high degree of central luminosity that gradually decreases towards the outer regions. A subtle color gradient is visible, with the central region appearing whiter, possibly indicating a population of older stars. The outer regions show a slightly bluer hue which may indicate lower levels of on-going star formation. No obvious spiral arm structure or prominent dust lanes are discernible in this image. There is no clear evidence of any recent major mergers, tidal tails, or significant morphological disturbances.
