The galaxy presents a generally elliptical morphology, appearing somewhat rounded in shape. The central region exhibits a significantly higher surface brightness, suggesting a prominent galactic nucleus or bulge. This central area is characterized by a yellowish hue, which could indicate an older stellar population. Extending outward from the core, the galaxy displays a less concentrated, diffuse halo. There is a subtle indication of a disk-like component, though it's not distinctly defined. The halo appears relatively smooth, lacking significant clumpy structures that would suggest ongoing major merger activity. Faint bluish regions are observed in the outer areas, possibly indicating the presence of younger stars and ongoing star formation, albeit at a subdued level. The galaxy's overall structure gives an impression of a system dominated by an older stellar population with a moderate amount of on going star formation, and a well-defined nucleus.