The galaxy presents a generally smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, indicating a possible bulge component. The overall shape is largely round, with a slight hint of deviation from perfect circularity. There appears to be minimal evidence of spiral arms or a well-defined disk structure, though there may be a hint of distortion in the lower portion of the galaxy. The galaxy's color is primarily a yellow-orange hue, which implies an older stellar population with reduced ongoing star formation. This is also supported by the redder z-band magnitude. There is no obvious indication of a major merger event, but some minor tidal disturbances cannot be ruled out based on the observed morphology. Based on the available data, the galaxy appears to be a relatively quiescent system.
