The galaxy appears as a somewhat elongated, disk-like structure oriented at an angle to our line of sight. Its color profile suggests a moderate amount of star formation activity. The central region of the galaxy presents a concentrated, yellowish hue, likely indicative of an older stellar population. Moving outward from the center, the galaxy's color shifts toward blueish and white tones, hinting at regions of active star formation. The presence of both older and younger stellar populations suggests ongoing stellar evolution within the galaxy. There is a hint of some disruption in the galaxy's shape, suggesting a possible recent or ongoing minor interaction with another galaxy. The galaxy's apparent size indicates that it is a fairly massive system. Overall, this appears to be a moderately active galaxy with signs of interaction.
