The galaxy presents as an elliptical-like structure, with a smooth overall appearance. The central region exhibits a concentrated, bright, yellowish hue, suggesting an older stellar population. Moving outward from the core, the color transitions to a bluer tone, particularly in the fainter regions. This color gradient indicates a potential shift towards younger stars or ongoing star formation in the outer parts of the galaxy, although the rate appears relatively low. The galaxy displays a somewhat elongated shape, deviating from a perfectly circular form. There is no visible evidence of strong tidal interactions or major disturbances affecting its morphology, though a subtle irregularity in the disk suggests some possible minor disturbances. The galaxy’s overall structure hints at a system that has undergone some degree of evolution and settling, with a mix of stellar populations and a relatively quiescent star-forming environment.
