The galaxy presents as a primarily smooth, elliptical-like structure. The core exhibits a high degree of luminosity, with a concentrated bright yellow hue suggesting a high density of older stellar populations. The light distribution appears to decrease steadily moving outwards. The outer regions show subtle deviations from a perfect elliptical shape, with some elongation visible. There are faint hints of possible disturbances in the outer regions, possibly indicative of a past or ongoing minor interaction or merger. However, there does not appear to be a major ongoing merger present. The overall color gradient suggests a relatively quiescent star formation rate.
