The galaxy presents as a moderately compact structure with an approximate radius of 3.7 arcseconds. The central region displays a somewhat smooth morphology, yet exhibits signs of disturbed features. Some faint, asymmetric extensions emanate from the core, suggesting a possible interaction or tidal disruption event. Color gradients are present with the core showing a slight shift towards redder wavelengths, potentially indicating an older stellar population, while the outer regions exhibit bluer hues, possibly indicative of more recent star formation. The galaxy's overall light distribution is not entirely uniform, hinting at some degree of structural complexity. It is difficult to definitively categorize the galaxy’s type given the apparent disturbances, but its core structure hints towards a disk-like formation. There is evidence of potential minor disturbances in the overall structure.
