This galaxy presents as a relatively smooth, elliptical-like structure. Its central region exhibits a bright, concentrated luminosity, indicating a likely dense stellar population within the galactic nucleus. The light gradually fades towards the outer edges, showing a decrease in stellar density. The overall shape appears quite round with a fairly simple form. The galaxy's color profile is somewhat uniform, hinting at a more homogeneous stellar population. The lack of prominent spiral arms or dust lanes supports the classification of a relatively quiescent galaxy with moderate star formation activity. There is no visual indication of a major ongoing merger, though there is a hint of a possible minor disturbance in the outer disk. Overall, the galaxy appears to be an early-type galaxy at a moderate redshift.
