The galaxy exhibits a generally elliptical morphology, although some disk-like features are present. There is evidence of some form of disturbance or interaction occurring, given the irregular distribution of light in the outskirts and the complex structure present. It appears to be a relatively massive system. The galaxy possesses a bright, concentrated core which may be indicative of an active galactic nucleus or a dense stellar population.

The light distribution suggests active or recent star formation, particularly in the bluer regions. It is likely to be an intermediate-redshift galaxy, with significant luminosity.