The galaxy presents as a luminous, roughly elliptical object. Its core region appears bright and concentrated, exhibiting a yellowish-white hue suggesting an older stellar population. Moving outwards from the center, the light gradually diminishes with a faint greenish tint. The overall structure seems smooth, lacking prominent spiral arms or distinct features typically associated with active star formation regions. However, there may be slight disturbances in its outer regions, possibly indicating interactions with smaller satellite galaxies or tidal effects. The galaxy's color profile, showing a gradual change from yellow to green as we move from the core to the outskirts, hints at a more complex stellar population distribution. It is likely undergoing low levels of star formation. The system does not show evidence of a major merger but may have experienced minor disturbance from a recent interaction.
