The observed galaxy presents as a diffuse, somewhat irregular structure. There's an apparent elongation along a primary axis, suggesting it's not perfectly spherical. The light distribution is uneven. A smoother, brighter central region, possibly indicative of a galactic bulge, is slightly offset within the galaxy's overall profile. The outskirts exhibit a clumpy and irregular structure, with several distinct, brighter condensations embedded within a fainter, more extended halo. These brighter knots appear bluer in color, suggesting recent star formation regions. Overall, the galaxy displays evidence of a possible interaction or merger event, given its disturbed morphology. The lack of a well-defined spiral arm structure or a smooth elliptical profile further supports the classification of an irregular galaxy potentially undergoing dynamic evolution.
