The galaxy presents an elliptical morphology, appearing largely featureless and smooth in texture. It exhibits a high degree of central concentration, with a bright core that dominates the overall luminosity. The light distribution gradually decreases outward from the core, forming a diffuse halo. The galaxy appears slightly elongated, with an axial ratio of approximately 0.7. There is no clear evidence of spiral arms, dust lanes, or ongoing star formation within the visible spectrum. Overall, this galaxy appears to be a relatively evolved system with a significant spheroidal component.
