The galaxy presents an elliptical morphology, appearing largely smooth in structure with no distinct spiral arms or bar-like features visible. The light distribution seems relatively uniform across the galaxy’s body, indicating a lack of significant ongoing star formation in well-defined regions. The color gradient suggests a possible older stellar population, exhibiting a slight reddish hue overall. There appears to be a faint halo extending beyond the main body of the galaxy, suggesting a population of sparsely distributed stars. There is no distinct nucleus visible, but that may just be due to image quality. There is no sign of any ongoing merging events.
