The galaxy appears to be elliptical in shape, exhibiting a smooth, relatively featureless morphology. Its light profile shows a strong central concentration, suggesting a significant bulge component. There is a gradual decrease in luminosity from the core outwards, with no distinct spiral arms or bar structures visible. The overall color is a slightly redder hue, hinting at an older stellar population and a relatively low rate of ongoing star formation. There is no evidence of any major disturbances or tidal features, which indicates that there have been no recent major merger events.
