The galaxy presents an elliptical morphology, with a smooth and centrally concentrated light distribution. The core exhibits a bright, yellowish hue, suggesting a population of older stars. There is a subtle elongation, the galaxy does not appear perfectly spherical, nor a cigar shape. There is no clear evidence of prominent spiral arms or a distinct disk structure. The galaxy appears relatively isolated, with no obvious signs of ongoing major mergers, but some disturbance cannot be ruled out. The light appears smoothly distributed and appears to be composed of mature stars. This galaxy exhibits characteristics consistent with a relatively evolved system, likely with a low star formation rate.
