The galaxy presents a roughly elliptical morphology, appearing more elongated than circular. It displays a smooth light distribution, with a central bulge that dominates the overall luminosity. The color gradient suggests a radial change in stellar population or dust content. The core of the galaxy exhibits a yellow-white hue, transitioning to a redder color in the outer regions. There is no obvious spiral structure or strong evidence of active star formation present in this image. The galaxy doesn't seem to be undergoing any major mergers, based on the lack of tidal tails or significant morphological distortions. It appears to be a relatively isolated system with a moderate size.