The galaxy presents as a centrally concentrated object, appearing relatively smooth in texture. There is a discernible elliptical morphology with a slight elongation. The core exhibits a bright, yellowish hue, which suggests a population of older stars, although some star formation is still present. Fainter, reddish, diffuse features extend from the central region, potentially indicating a low level of on-going star formation in the outer regions or dust lanes. There's a hint of disturbance within the extended halo structure, although without further spectral analysis, we can only speculate on the nature and cause of this irregularity. The overall color profile suggests a more evolved system.
