The galaxy presents as a slightly elongated, centrally concentrated object. The core region exhibits a yellow-white hue, indicative of an older stellar population. Surrounding the core, the galaxy transitions to a bluer color, implying the presence of younger, hotter stars in the outer regions. The overall light distribution appears relatively smooth, without prominent spiral arms or distinct morphological features. There's a subtle color gradient with radius, the outer regions possessing a slightly more bluish tint, potentially indicating ongoing star formation. No signs of significant tidal disturbances or ongoing major mergers are apparent, though a minor asymmetry or subtle distortion can not be ruled out. The overall appearance suggests a galaxy that is relatively evolved, possibly transitioning from active star formation to a more quiescent state.
