The galaxy presents as a relatively small, edge-on spiral or lenticular galaxy. A central bulge is visible, appearing brighter and more concentrated than the surrounding disk. There is a slight color gradient observed, with the central bulge exhibiting a yellowish hue and the outer disk regions showing hints of bluer light. The disk appears smooth, without any obvious spiral arm structures or prominent dust lanes visible at this resolution. The morphology suggests a relatively evolved system with a significant spheroidal component and a flattened disk. It is possible that the galaxy is undergoing a period of quiescence with suppressed star formation, indicated by the dominance of older stellar populations in the central bulge and the lack of prominent HII regions. The slight color gradient and smooth disk structure imply a relatively undisturbed evolutionary history without significant recent merger events.
