The galaxy presents as a centrally concentrated, generally smooth object with a high degree of circular symmetry. There is no apparent spiral arm structure or distinct morphological features such as bars or rings. A significant fraction of the galaxy's light appears concentrated in a central bulge or core, indicating a high stellar density in this region. The color gradient suggests the presence of a dominant older stellar population. The galaxy's overall color appears more red than blue, which may signify a lower rate of recent star formation compared to other galaxy types. Based on the evidence, this galaxy is most likely an elliptical.
