The galaxy presents a generally smooth and rounded morphology, exhibiting a concentrated central bulge with a yellow-orange hue, indicative of an older stellar population. Fainter, somewhat diffuse disk-like features extend from the bulge, with subtle hints of bluer star-forming regions particularly along one edge. There is also a hint of potential gravitational disturbance in the form of a very slight tail and one slightly disturbed arm. Although these are not a clear indication of merging, they are worth noting. There appears to be a relatively high degree of central concentration, and the overall light profile suggests a considerable stellar mass. Based on the colors and features, it seems this galaxy may be in the process of transitioning from a more active, star-forming state to a more quiescent one.
