The galaxy presents as a somewhat diffuse, irregular object. There is a brighter, more condensed region that may be indicative of a central bulge or a region of enhanced star formation. The overall morphology suggests a relatively evolved system, though signs of past or ongoing interaction cannot be ruled out. There is a strong chance of a recent merger event based on visual irregularities. The light profile appears to be relatively smooth, but is difficult to definitively characterize due to limited resolution. Based on the slight color variation, there is a possibility of ongoing star formation. It appears to be a relatively massive galaxy with a moderate rate of star formation. The object is likely located at a significant cosmological distance, based on its apparent size and measured properties.
