The galaxy presents as a moderately sized object with an apparent semi-major axis of under 2 arcseconds. The galaxy's morphology is predominantly smooth. There is a slight indication of a disk-like component, but it is less pronounced compared to the smooth central region. The overall shape is fairly round, exhibiting minimal elongation. There are notable disturbances in the galaxy's structure. The presence of these features suggest there may be a potential ongoing or recent merger event. Color analysis indicates that the object appears brighter in redder wavelengths compared to bluer wavelengths. The overall characteristics suggest a galaxy undergoing some form of interactive process, potentially affecting its morphology and stellar populations.
