The galaxy presents as a generally elliptical form, appearing more elongated than circular. The central bulge is prominent and exhibits a yellowish hue, suggesting an older stellar population.  Moving outward from the core, the color transitions subtly to a slightly greenish-yellow disc, indicating the presence of a younger, though likely still subdued, star formation region. The overall light distribution is smooth with no clear signs of spiral arms or distinct morphological features. Minor disturbances are potentially present, though difficult to ascertain given the image resolution, suggesting an absence of major merger activity.
