The galaxy appears to be relatively compact and exhibits an irregular morphology. The central region shows a bright, concentrated core, possibly indicating an active galactic nucleus or a region of intense star formation. Surrounding this core, the light distribution is uneven, suggesting a disturbed or disrupted structure. There are hints of tidal features or faint extensions, possibly indicating a recent or ongoing merger event. The galaxy has an overall bluish hue, suggestive of a younger stellar population and ongoing star formation activity. There is some indication of dust absorption in the galaxy as well.
