The galaxy presents as a centrally concentrated object with an overall smooth morphology. The core region exhibits a bright, yellowish-white hue, suggesting a population of older stars. The outer regions display a less intense, somewhat bluish coloration on the left side, hinting at the presence of younger stellar populations or perhaps ongoing star formation, but this cannot be said with certainty. The galaxy appears to be largely spheroidal, showing a high degree of roundness. There is no clear evidence of strong spiral arm structure or a significant disk component from the image alone. Subtle irregularities in the outer regions suggest the possibility of minor interactions or past merger events, but the dominant impression is one of a relatively undisturbed, evolved system. The galaxy exhibits a low degree of internal complexity based on the color gradients and absence of significant sub-structures.
