This galaxy exhibits a generally smooth morphology, with an overall shape that is intermediate between round and elongated. There is evidence of possible tidal disruption, with faint bluer light extending from the main body of the galaxy in what appears to be a tidal tail or stream. The main body displays a significant concentration of older stars, as evidenced by its yellow/orange color. This suggests that the star formation rate in the core may be suppressed. The size of the galaxy appears relatively compact. Overall, the galaxy appears to be in a state of merging or recent interaction.
