The galaxy exhibits a generally elliptical morphology, appearing somewhat elongated or cigar-shaped. The central region shows a brighter, more concentrated luminosity, suggesting a significant stellar density. Progressing outwards from the center, the light gradually diminishes, with fainter, bluer hues becoming more pronounced. The galaxy appears relatively smooth in structure, without any prominent spiral arms or obvious irregular features, which are more common in spiral galaxies. There is only subtle variation in the color profile from the central region to the outer regions.
