The galaxy appears to be an elliptical galaxy, characterized by a smooth, nearly featureless light distribution. It exhibits a concentrated central bulge, with the light intensity decreasing gradually outwards. The overall shape approximates a circular morphology, showing a high degree of rotational symmetry. The color of the galaxy is predominantly yellow-orange, suggesting an older stellar population dominated by evolved stars. There is no apparent evidence of significant spiral arm structure or prominent dust lanes. No signs of major disturbances or ongoing mergers are immediately obvious, suggesting a relatively quiescent state.
