The galaxy appears as an elliptical or lenticular system, exhibiting a smooth, relatively featureless morphology. Its light profile suggests a concentrated central bulge, potentially indicative of an older stellar population with minimal ongoing star formation. The galaxy presents a yellowish hue, which may reflect a dominance of older, redder stars. There is evidence of a possible interaction or minor disturbance, perhaps due to a smaller companion galaxy in the vicinity, although its form is generally unperturbed. The system's moderate roundness indicates a possible departure from a perfect elliptical shape.
