The galaxy presents an overall elliptical morphology, appearing largely smooth in texture. A significant portion of the galaxy's light is concentrated in a central bulge, exhibiting a yellowish hue, indicative of an older stellar population. There is evidence of a potential merger event. The main body of the galaxy has some subtle disturbances, and two distinct luminous clumps are visible, which may indicate the presence of interacting galactic nuclei or regions of intense star formation triggered by the merger. There are no immediately apparent spiral arm structures or significant dust lanes visible. The general roundness of the object suggests a relatively low inclination angle with respect to our line of sight.
