The galaxy appears to be a relatively large, early-type system at a redshift of approximately 0.3. It exhibits a predominantly smooth morphology, with a bright central region indicating a concentrated nucleus. The light distribution is largely spheroidal, although there are some hints of a disk-like structure or possibly a merging event with minor disturbances.

The galaxy displays a color gradient, appearing bluer in the outer regions and redder towards the center. The star formation is currently low but not absent. There is a very slight asymmetry to the overall shape, suggesting that some minor interaction could be taking place. The majority of visible stars are present in the brighter central nucleus of the galaxy.
