The galaxy presents as a relatively smooth, elliptical-like structure, although some disturbance is apparent. It exhibits an overall elliptical shape but lacks a defined spiral arm structure. The color profile indicates a potentially older stellar population, with a dominant redder hue, but some star formation may be occurring as the galaxy also exhibits a slightly greener color. The galaxy seems to be in the process of a merger event, possibly with multiple smaller galaxies as there are multiple blobs of light. The galaxy core appears somewhat irregular. There are multiple areas of distinct brightness throughout the galaxy, indicating heterogeneous mass distribution.
