The galaxy presents as a somewhat elliptical structure, appearing mostly smooth in texture with a slight elongation along its major axis. The central region exhibits a concentration of luminosity, suggesting a possible bulge. A subtle color gradient is observed, transitioning from a relatively bluer hue in the outer regions to a more yellow-red color towards the center. This implies potential variations in stellar populations, with the presence of younger, bluer stars in the periphery and older, redder stars concentrated in the core. There is a hint of a disk-like structure, although it is not well-defined. No significant signs of ongoing major merger activity or tidal disturbances are apparent. The overall morphology leans towards that of an early-type spiral galaxy.
