The galaxy presents a largely smooth, elliptical morphology. It exhibits a bright, concentrated central bulge that dominates its overall structure. The overall color appears to be on the bluer end of the spectrum, suggesting the potential presence of younger stellar populations and ongoing star formation, although it could be intrinsically blue.  There is a very faint hint of a possible disk, viewed almost edge-on.  A very slight deviation from a perfectly elliptical shape may suggest a minor gravitational interaction, such as a past or ongoing minor merger, but the morphology is mostly undisturbed. The galaxy exhibits a relatively high degree of central concentration, with the luminosity declining smoothly towards the outer regions. The size is relatively compact.
