The galaxy exhibits a primarily smooth morphology, with a centrally concentrated, bright core. The light distribution appears relatively symmetrical and rounded, indicative of an elliptical galaxy or a spiral galaxy viewed face-on without prominent spiral arms. There is a suggestion of a fainter, extended halo surrounding the central region. The color gradient transitions from an orange hue in the central region to a more yellow-greenish hue in the outer regions. This color suggests an older stellar population dominating the core, with a possible contribution from younger stars in the outer halo, though the difference is subtle. There is no clear evidence of significant dust lanes or active star-forming regions readily apparent in this image. The overall appearance suggests that this is an older, relatively evolved galaxy.
