This galaxy exhibits a generally smooth morphology, suggesting it is likely an elliptical or lenticular galaxy. There is little evidence of spiral arms or prominent disk features. The light distribution appears concentrated towards the center, and the galaxy presents an approximately round shape, with some deviation. There is little to no indication of significant ongoing merger activity or major disturbances in its structure, although some minor irregularities cannot be ruled out. Based on the color profile, the stellar population appears older, with lower recent star formation, consistent with a more evolved system.
