The galaxy presents as a centrally concentrated object, exhibiting a smooth, largely featureless morphology. The light distribution is centrally dominant, with a gradual falloff in surface brightness towards the outer regions. The color profile appears relatively uniform, trending towards redder hues, particularly in the central region, suggesting an older stellar population. There is no apparent spiral structure or distinct dust lanes visible. The galaxy appears fairly round in shape, exhibiting a high degree of axial symmetry. There is no visually discernible evidence of ongoing merger activity or significant tidal disturbances, though minor disturbances cannot be ruled out at this resolution. The galaxy's overall appearance suggests a relatively quiescent system, potentially an elliptical or lenticular galaxy.
