The galaxy appears as a central bright and smooth spheroid, likely a bulge component. The light is concentrated, indicating an older stellar population with minimal dust obscuration. There is a slight extension that may represent a disk component, however it is much less prominent than the bulge and also appears smooth. The overall color is consistent with a galaxy that has undergone significant quenching of star formation in the recent past. The colors are slightly bluer in the core than further out suggesting that any ongoing star formation is centrally concentrated. There is a slight asymmetry observed in the galaxy's structure, which could be due to a minor gravitational interaction or recent merger event. The lack of defined tidal tails suggests that this interaction occurred some time ago, allowing the galaxy to settle back into a relaxed state. Overall, the galaxy seems to be a lenticular type with a slight chance of recent or current gravitational disturbances.
