The galaxy presents a primarily elliptical morphology, although there is subtle evidence of a disk-like structure. The central bulge is prominent, exhibiting a concentrated brightness and yellowish-orange hue. There is a gradual decrease in surface brightness from the core towards the outer regions. The overall color suggests a relatively old stellar population, potentially indicating a lower ongoing star formation rate within the galaxy. There is no obvious strong evidence of spiral arms or significant dust lanes. There is a slight irregularity to the galaxy's shape, which could possibly indicate a minor gravitational interaction.