This galaxy appears to be a relatively smooth, centrally concentrated system. The light profile suggests a possible elliptical or lenticular morphology, although there is a hint of a disk-like structure present. The central region is characterized by a bright, concentrated core, which may indicate the presence of an active galactic nucleus or a dense stellar population. The galaxy exhibits a slightly bluer color in its central regions transitioning to redder colors towards the outer edges, potentially indicating ongoing star formation within the nuclear region or a difference in stellar population. There are hints of possible minor disturbances in the galaxy's structure, potentially due to a minor merger event. Overall, the galaxy seems to be a relatively evolved system with moderate star formation activity.
