The galaxy appears to be an elliptical galaxy, characterized by a smooth, concentrated light distribution. It exhibits a spheroid-like morphology. The color profile is dominated by yellowish hues, suggesting a population of older stars with lower rates of on-going star formation. There is no evidence of spiral arms or a prominent disk structure. The galaxy shows a moderate ellipticity, appearing somewhat elongated rather than perfectly spherical. There are no clear signs of major mergers or tidal disturbances. The galaxy seems relatively isolated and unperturbed.
