The galaxy presents a generally elliptical morphology, appearing largely smooth and featureless in this image. The central region exhibits a brighter, more concentrated luminosity, suggesting a higher density of stars. Moving outward from the core, the light gradually diminishes, forming a diffuse halo. A subtle color gradient is observable, transitioning from a warmer, yellowish hue in the center to a cooler, bluish tinge in the outer regions. There's no indication of significant spiral arm structures or active star-forming regions. The galaxy appears relatively undisturbed, with no obvious signs of ongoing or recent merger activity. Its overall shape leans towards an intermediate ellipticity, positioned somewhere between a perfectly round form and a more elongated, cigar-like appearance.
