The galaxy appears as a centrally concentrated object, displaying a generally smooth morphology. There is some indication of a slightly elongated shape. The central region exhibits a yellowish-white hue, suggesting an older stellar population. Moving outward from the core, the color transitions to a faint greenish-blue halo. The overall structure suggests a likely elliptical galaxy type. Evident from the images is the lack of any prominent spiral arms or a well-defined disk structure. The galaxy does not show evidence of any significant ongoing merger activity or tidal disturbances.
