The galaxy presents a generally smooth, elliptical morphology. It exhibits a notable concentration of light towards the center, suggesting a prominent galactic nucleus. The galaxy appears relatively regular in shape, with a slight elongation that deviates from a perfectly circular form. The color distribution shows a central yellowish hue, potentially indicative of an older stellar population, transitioning to slightly bluer tones in the outer regions. This color gradient might suggest ongoing, albeit moderate, star formation activity within the galaxy's disk. There is no strong evidence of significant disturbances or major mergers in this image. Faint outer features appear relatively undisturbed, but further analysis is required to confirm its detailed morphological classification.
