This galaxy appears to be of relatively small angular size. It exhibits a somewhat amorphous morphology, lacking a well-defined spiral structure or elliptical shape. The light distribution appears centrally concentrated, with a decrease in intensity towards the outer regions. It demonstrates a relatively smooth light profile overall, however it is disrupted and has some features of possible minor disturbance. There is an indication of a slight elongation or irregularity in its shape, which could be indicative of gravitational interaction or internal processes. There may be some level of recent or ongoing star formation. There appears to be no obvious major merger.
