The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The core exhibits a yellowish-white hue, suggesting an older stellar population. Moving outwards from the core, the color shifts towards a bluish tint, potentially indicative of younger, hotter stars or ongoing star formation within the galaxy's disk. The galaxy's overall shape appears somewhat rounded, although there is a subtle elongation suggesting it may not be perfectly spherical. There is no clear evidence of major tidal disturbances or ongoing merging events, although a slight irregularity in the outer regions hints at possible minor interactions. Overall, the galaxy seems to be a relatively massive system, with a moderate amount of star formation.
