The galaxy presents a generally smooth, elliptical morphology. Its core appears intensely luminous and exhibits a yellowish hue, suggesting a population of older stars. A gradual decline in luminosity is observed as one moves from the core to the outer regions. The surrounding halo exhibits a subtle bluish tint, hinting at the presence of younger, hotter stars or ongoing, albeit moderate, star formation. There is no evidence of prominent spiral arms, bars, or other distinct morphological features typically associated with disk galaxies. The overall structure is suggestive of an evolved system, potentially with past merger activity that has contributed to its smooth, spheroidal appearance. There are no obvious signs of ongoing major mergers or tidal disturbances.
