The galaxy presents as a relatively smooth, elliptical morphology. The central bulge is prominent and appears luminous, displaying a yellowish-white hue. The outer regions of the galaxy show a gradual decrease in surface brightness, fading into the background sky. There is subtle evidence of a flattened disk component, though the galaxy lacks well-defined spiral arms or prominent dust lanes. The overall color profile suggests a stellar population dominated by older stars, with limited ongoing star formation. The galaxy shows some evidence of possible minor interaction or disturbance, such as an irregular feature or a slight warp in the disk.
