The galaxy presents a primarily smooth and rounded morphology. There is a slightly brighter central bulge. The disk appears featureless, with no clear spiral arm structures discernible. The color distribution suggests a higher concentration of older stellar populations, particularly within the bulge. The lack of distinct features and relatively smooth light profile could indicate a relatively quiescent or post-starburst system. There is a subtle elongation or flattening effect indicating the object is not perfectly circular, leaning towards a more elliptical shape. There is a hint of blue emissions in the outer regions, suggesting a small level of recent star formation, although it is not obvious. There is no evident signs of tidal disturbances or active galactic nuclei, but the image resolution limits any such conclusions. There are no nearby galaxies that suggest a merging event is actively occurring, or that the object is a result of recent merger events.
