The galaxy presents an overall elliptical morphology, although some irregular features are apparent. The central region exhibits a higher surface brightness with a yellowish hue, suggesting an older stellar population. Moving outward from the center, the color transitions to a bluer tint indicating more recent star formation, particularly on the left side of the galaxy. There appears to be a tidal tail extending from the upper right of the galaxy; this tail is composed of a distinct red region which could be due to H-alpha emission as a result of star formation. The overall structure suggests the galaxy may have undergone, or is currently undergoing, an interaction or minor merger event.
