The galaxy presents as a generally smooth, elliptical-like object with a concentrated central bulge exhibiting a yellowish-white hue, indicative of an older stellar population. Moving outwards from the core, the galactic disc has a slight blueish tinge, particularly in the outer edges, potentially implying some ongoing star formation, although this is not distinctly apparent. There are no visible spiral arm structures or bar features. The overall morphology suggests a galaxy that has largely completed its major mergers, residing at a distance where the light is redshifted by a factor that places it at an intermediate distance. Its mass falls within the realm of a large galaxy, and exhibits a moderate amount of star formation. The symmetry and lack of significant disturbances suggest that it is an evolved system that has not experienced a major merger recently.
