The galaxy presents a generally smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, indicative of a high degree of bulge dominance. There are no readily apparent spiral arm structures or significant dust lane features visible in the image. The color profile appears relatively uniform across the galaxy, transitioning from a more intense yellow core toward the outer edges where it is lighter. Minor irregular morphological features cannot be ruled out, as the image resolution limits detailed analysis. No obvious signs of ongoing major merger activity or strong tidal disturbances are immediately present. Given the overall morphology and color characteristics, a classification towards the early-type end of the Hubble sequence seems appropriate.
