The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears more yellow-orange in color, suggestive of an older stellar population dominating the core. This color gradually fades toward the outer regions of the galaxy, where bluer hues are subtly visible, indicating some presence of younger stars. The overall morphology suggests a system that has largely undergone its major star formation epochs, with ongoing star formation occurring at a lower rate. There is no obvious spiral arm structure. The galaxy appears largely undisturbed, showing no major signs of merging or tidal interactions. The roundness and lack of strong features implies that the galaxy has not experienced a major disturbance for some time.
