The galaxy presents an elliptical morphology, appearing largely smooth with a dominant central bulge. The galaxy exhibits a concentrated luminosity profile. There is a possible slight asymmetry visible, perhaps indicating a minor gravitational interaction or disturbance. There is an indication of some star formation activity within the disk, although at a modest rate. The galaxy's overall color suggests a population of intermediate to old stars. It is likely a massive galaxy, possibly at a distance where detailed morphological features are difficult to resolve with this image resolution. The galaxy does not appear to be undergoing a major merger, although a possible minor interaction can't be ruled out. The shape appears to be elongated, but not extremely so.
