This galaxy appears to be a relatively bright object with an estimated angular size of approximately 4 arcseconds. Morphologically, it presents as a system undergoing or having undergone a merger event. There is a prominent central bulge exhibiting a yellowish hue suggesting an older stellar population. Fainter, bluer regions are observed extending outward from the central bulge, potentially indicating areas of more recent star formation. The overall shape is irregular, deviating significantly from a typical elliptical or spiral morphology. This suggests gravitational disturbances are present, potentially due to the ongoing or recent interaction with another galaxy. Some distortion of the main body is visible, with a suggestion of tidal tails or disrupted arm structures, although the image resolution limits definitive identification.
