The galaxy presents as a centrally concentrated, luminous object with an overall elliptical morphology. It exhibits a smooth appearance, with no readily apparent spiral arm structure or significant dust lanes visible at this resolution. The central bulge is prominent and displays a yellowish-orange hue, suggesting a population of older, redder stars. The outer regions of the galaxy are less concentrated and appear bluer in color, possibly indicating the presence of a younger stellar population and ongoing star formation, although at a relatively low rate. There is some evidence of minor disturbances to the shape, possibly caused by gravitational interactions with a nearby object or a previous minor merger event. The galaxy displays an intermediate degree of roundness.
