The galaxy appears as a centrally concentrated object, likely an elliptical galaxy given its apparent smooth light distribution. There may be a small hint of a disk-like structure or spiral arms, but this is unlikely given the data. The galaxy has a somewhat rounded, slightly elongated shape. The luminosity is concentrated towards the center, with a gradual decrease in brightness moving outwards. The core of the galaxy appears very bright and yellowish-white, while the outer regions have a redder color. There appears to be no significant dust lane obscuring the central region. The galaxy does not appear to be undergoing a major merger, although there is a minor possibility of some tidal disturbance. There is also the possibility that the galaxy image has some artifacting.
