This galaxy appears to be undergoing some form of interaction or disturbance. The morphology suggests it is not a purely elliptical or spiral type, but exhibits features indicating a possible merger or tidal interaction. There is an extended halo of faint light surrounding the central region. Two distinct bright regions are observed. One is slightly redder in color, and the other is bright blue. This blue area may be due to strong star formation. There is also a fainter tail-like or plume-like feature extending outwards, which could be evidence of a tidal tail formed during an interaction with another galaxy, or perhaps a recent merger event. The light distribution appears somewhat asymmetrical, further supporting the idea of an ongoing or recent interaction.
