This galaxy appears to be a relatively smooth, elongated system. Its light profile suggests a spheroidal shape, potentially an elliptical galaxy or a lenticular galaxy viewed at an angle. The core exhibits a yellowish hue, which could indicate an older stellar population dominating the central region. Fainter blueish structures are present in the outer regions. The lack of pronounced spiral arms or dust lanes supports the classification of the galaxy as elliptical or lenticular. Overall, this galaxy exhibits characteristics consistent with a galaxy that is evolving slowly.
