The galaxy presents a generally smooth and rounded morphology. It displays a concentrated central bulge, which appears yellowish-white, indicative of an older stellar population. Surrounding the bulge is a fainter, bluish halo. There is some subtle unevenness to the halo, but no clear spiral arm structure or dust lanes are visible. The galaxy appears relatively isolated and undisturbed, with no obvious signs of a major ongoing merger, although some minor disturbances may be present. Overall, the galaxy appears consistent with an elliptical or S0 type galaxy, observed at a moderate distance.
