The galaxy appears as a lenticular or possibly elliptical system, displaying a smooth, featureless morphology. It exhibits a moderately elongated shape. There is a subtle indication of a disk-like structure, but it is not distinctly spiral. There is little evidence of major disturbances or merging events, though minor disturbances cannot be entirely ruled out. The galaxy displays a magnitude which is relatively bright, suggesting a substantial stellar population and ongoing star formation within the galaxy, though at relatively low levels. Overall, it appears to be a fairly well-formed galaxy undergoing a period of relatively quiescent evolution.
