The galaxy presents an overall elliptical morphology, appearing smooth and relatively featureless. It exhibits a notable central bulge, concentrated and bright, suggesting a high stellar density and likely dominated by older stellar populations. The galaxy displays a color gradient, transitioning from a yellowish-white core to a bluer hue in the outer regions. This color difference potentially indicates a shift in stellar populations, with older, redder stars prevalent in the center and younger, bluer stars present in the outskirts. There are hints of a subtle disk-like structure viewed at an angle, as the galaxy is somewhat elongated, rather than perfectly spherical. The lack of prominent spiral arms or dust lanes supports the classification as an early-type galaxy, with a relatively low ongoing star formation rate. Minor disturbances appear to be impacting the structure of the galaxy.
