The galaxy presents a centrally concentrated luminosity profile, with the light appearing to diminish gradually with increasing radius. The core exhibits a bright, almost unresolved, point-like nucleus, indicative of possible active galactic nucleus (AGN) activity. The overall color is bluish-white, suggesting a stellar population with a notable presence of young, hot stars and ongoing star formation. Around the galaxy, there is a faint, diffuse halo of light, extending further than the brighter central region. This halo has subtle irregularities and a slight elongation, possibly hinting at past minor interactions or tidal disturbances. However, there are no clear signs of major mergers or strong tidal tails, suggesting the galaxy is either undisturbed or is in the late stages of assimilating smaller companions. There are some possible wisps or dust lanes visible in the disk but the overall impression is relatively smooth. 
