The galaxy exhibits a generally smooth morphology, with a high degree of central concentration. Its light profile transitions gradually from a bright, yellowish-white core outwards. The shape of the galaxy appears slightly elongated, but not strongly so; it is more ellipsoidal than disk-like. There is faint indication of a possible tidal feature or minor disturbance, perhaps suggesting a past or ongoing interaction with a smaller companion. Based on the light detected, there appears to be low star formation activity. The galaxy is likely a massive system given its luminosity and the presence of an older stellar population contributing to its smooth appearance.
