The galaxy presents a largely smooth and centrally concentrated morphology. It appears nearly round with only subtle deviations from perfect circularity. The core exhibits a bright, condensed region, indicative of a significant concentration of stars or potentially an active galactic nucleus. There's a gradual decrease in luminosity from the center outwards, suggesting a relatively homogenous stellar population and a lack of prominent spiral arms or distinct features such as dust lanes. There is very little sign of recent merger activity or disturbances. Faint, diffuse light extends outwards from the central core, indicating the presence of an extended stellar halo. Overall, the visual characteristics of this galaxy suggest it is likely an elliptical galaxy or a lenticular galaxy viewed face-on. It appears to be in a relatively quiescent state, with minimal signs of ongoing star formation or significant interactions with other galaxies.
