The galaxy presents a generally elliptical morphology, appearing elongated but significantly lacking in distinct spiral arm structures. The central bulge exhibits a high surface brightness, suggesting a dense concentration of stars. The color gradient transitions smoothly from a yellowish-white core to a fainter, slightly bluer outer region. This color difference may indicate ongoing star formation in the galaxy's periphery, though at a low rate.

The galaxy's overall structure appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. Subtle asymmetries are present, possibly indicative of minor disturbances or past accretion events, but without a high degree of certainty.
