The galaxy presents a generally smooth appearance, suggesting an elliptical morphology or a spiral galaxy seen face-on with a dominant bulge. It exhibits a central concentration of light that fades gradually outwards. Its overall shape is elongated, with the major axis being roughly three times the length of the minor axis. There is a subtle color gradient across the galaxy, transitioning from a yellow-orange hue in the core to a redder tone in the outer regions. There are no obvious spiral arm features or signs of recent major merging events. The relatively smooth appearance and color profile suggest a galaxy with an older stellar population and a lower ongoing star formation rate. There is a slight indication of minor disturbances in the form of subtle asymmetries in the outer regions.
