This galaxy exhibits a generally smooth morphology, with a predominantly elliptical shape. The light distribution appears concentrated towards the center, suggesting a prominent bulge. There are no clearly defined spiral arms or distinct disk-like features visible in this image. The color profile indicates a potential mix of stellar populations. The central region displays a bluer hue, which could be indicative of younger, hotter stars and ongoing star formation activity. The outer regions show a redder tint, suggesting older, cooler stellar populations. Overall, this galaxy presents as a relatively evolved system, with some evidence of recent or continued star formation, yet lacking significant disturbances or merging activity in the immediate vicinity. The galaxy displays an intermediate roundness.
